The galaxy presents as a roughly elliptical, relatively smooth object. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or active galactic nucleus. Moving outwards from the center, the luminosity gradually decreases, with no distinct spiral arm structures visible. The overall color profile appears somewhat red, indicating a population of older stars. Slight asymmetry is apparent in the outer regions. There are no signs of tidal tails or obvious merging activity suggesting it is not undergoing major interactions.

