The galaxy presents a roughly elliptical morphology, appearing as a moderately luminous and centrally concentrated object. The light distribution is predominantly smooth, with the central region exhibiting a bright, almost unresolved core suggestive of a potential active galactic nucleus or a dense stellar population. Fainter, diffuse extensions are visible, hinting at a possible disk or tidal features.

The color profile indicates a mixture of stellar populations. The core appears bluer, consistent with ongoing star formation or a younger stellar population. Surrounding the core, the colors shift towards a more yellow/red hue. The overall color suggests a system with moderate star formation activity but also a significant population of older, redder stars. There is evidence of some disturbance and possibly a merging event, or minor tidal interactions. The overall light profile is relatively compact, indicating a moderate size.
