This galaxy presents as a somewhat elliptical structure with a dominant central bulge. The light profile appears smooth, transitioning from a bright, concentrated core to a more diffuse halo. The color is generally reddish-orange, suggesting a population of older stars. Subtle irregularities in the outer regions may be indicative of minor disturbances or ongoing interactions, although there are no obvious signs of a major merger. The galaxy appears to be relatively massive with suppressed star formation.
