The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is centrally concentrated, exhibiting a gradual decrease in luminosity towards the outer regions of the galaxy. The core appears yellowish-white, suggesting a population of older stars dominating the central region. The outer regions show a subtle shift towards redder hues, further supporting the presence of an aging stellar population. No distinct spiral arms or significant dust lanes are discernible. There are hints of very faint extensions around the central region, but these are subtle and do not suggest an actively merging system. The overall shape appears close to circular. There is a hint of distortion on the right side, but it doesn't appear to be a clear indication of a major merger. 