This galaxy presents a complex morphology, exhibiting features suggestive of an ongoing or recent interaction or merger event. The central region displays a concentrated, bright core, which appears yellowish in color, indicating a population of older stars.

Extending outwards from the core, a disturbed disk-like structure is visible. This structure shows signs of asymmetry, with a bluer region apparent on the lower side of the galaxy, potentially indicating younger stellar populations and active star formation. The overall light distribution is not uniformly smooth; instead, it shows several distinct clumps and extensions, which is consistent with a disturbed system.

There is an indication of a possible tidal tail or plume extending from the central part. The galaxy does not exhibit a clear spiral arm structure, suggesting that the morphology has been significantly disrupted. The luminosity profile seems to indicate this is a massive galaxy experiencing a relatively low rate of star formation in a mature galaxy, which is not unusual. The overall color gradients suggest a spatial variation in stellar populations, possibly resulting from the merger dynamics.
