The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated morphology. It exhibits a subtle elongation, deviating slightly from a perfectly round shape. The color profile suggests a dominant older stellar population, as evidenced by the yellowish-white hue in the core region. There might be some very low-level recent star formation towards the edges, indicated by very faint hints of bluer tones, but overall the galaxy is dominated by older stars. There is no prominent evidence of strong spiral arms, a well-defined disk structure, or significant dust lanes within this galaxy. Furthermore, there are no obvious signs of tidal disturbances or ongoing mergers. The overall impression is that of a relatively isolated galaxy, in a relatively relaxed state.
