The galaxy presents as a somewhat elliptical structure. Its central region exhibits a bright, concentrated luminosity suggesting a high density of stellar population. The color profile appears to be on the redder side, especially in the core, indicating an older stellar population and/or significant dust obscuration. Fainter, bluer light is present in a few areas, possibly indicating younger stars or star forming regions.

The galaxy appears to be a relatively smooth structure, but with a hint of asymmetry or faint disk-like structure. There may be minor tidal disturbances present but it's difficult to tell. It does not appear to be undergoing a major merger.
