The galaxy presents a roughly elliptical morphology, though the structure is not perfectly smooth. There is evidence of some disruption in the overall light distribution, potentially indicating an interaction or internal dynamics. The central region displays a slightly brighter and more condensed appearance. A slight extension is visible along the major axis, which could point to a faint disk component or tidal feature. The color profile suggests a population of older stars, as the galaxy exhibits a reddish hue overall. There are faint, diffuse features that may be indicative of tidal tails or plumes, suggesting possible minor merger activity in its past. However, the majority of the light is concentrated in the central region, giving the galaxy an appearance of being generally undisturbed.
