The galaxy appears to be an elliptical system, characterized by a smooth, centrally concentrated light distribution. It exhibits a generally round morphology, with a slight elongation suggesting a possible oblate spheroid shape rather than a perfect sphere. There is no distinct disk structure visible, and the galaxy lacks prominent spiral arms or bar features. The dominant color is whitish-yellow, with a subtle bluish-white hue concentrated towards the core. This color gradient suggests that the central region may host a population of younger, hotter stars compared to the outer regions, although the overall stellar population is likely dominated by older stars, indicative of an evolved system with relatively low ongoing star formation. There is no evidence of recent major merger events or significant tidal disturbances. Close inspection does not reveal any distinct dust lanes. Overall, this galaxy presents as a relatively quiescent elliptical galaxy, likely residing in a relatively low density region of space.
