The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that dominates the overall light profile. Faint, diffuse extensions are visible, suggesting a stellar halo surrounding the main body of the galaxy. The galaxy's shape is slightly elongated. The color of the galaxy appears to be yellow-white, indicative of a stellar population dominated by older, lower-mass stars. There are also regions of redder color, which may indicate the presence of dust or a population of older stars. No distinct spiral arms or active star formation regions are observed. The galaxy appears to be isolated, with no obvious signs of tidal interactions or recent mergers.
