The galaxy presents as a relatively smooth, elliptical form with a distinct central bulge. The core appears luminous with a yellow-white hue, suggesting a population of older stars. Moving outward from the core, a bluer halo is visible. This might indicate a lower density of stars or a more recent star formation. The galaxy exhibits a slight elongation, but mostly seems to be circular. There is no apparent strong tidal distortion suggesting it is not currently undergoing a major merger, although there may be minor disturbances present in the outskirts. Overall, it is a moderately massive galaxy with ongoing star formation.
