The galaxy presents as a fairly regular, smooth object with a generally elliptical morphology. The light distribution appears relatively uniform across its surface, suggesting a lack of significant spiral arm structure or prominent dust lanes. Color gradients across the galaxy are subtle, though the central region appears slightly redder than the outer regions. This color difference may indicate an older stellar population concentrated towards the galactic core, with ongoing, but low-level star formation. There's no evidence of strong tidal features or morphological distortions, implying it is unlikely undergoing a major merger event. Given its smooth appearance, it appears to be a relatively evolved system.
