This galaxy presents as a relatively smooth object, exhibiting a notable concentration of light towards its central region. The overall form approximates a flattened spheroid, though it deviates noticeably from perfect circularity. There is evidence of faint, diffuse extensions beyond the main body, hinting at a possible extended halo or tidal features, though these are not sharply defined. A color gradient is present, with bluer hues dominating the core and inner regions, transitioning to redder tones in the outer parts. This suggests ongoing star formation in the center, with an older, redder stellar population more prevalent in the periphery. There may be minor disturbances to the galaxy, as it does appear to be a merging galaxy.
