The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated morphology. It appears elongated, with the major axis significantly exceeding the minor axis. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region, indicating a paucity of ongoing star formation. The galaxy lacks any readily discernible spiral arm structures or prominent dust lanes. There is no evidence of any major mergers or significant tidal disturbances. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards.
