The galaxy presents as a relatively smooth, centrally concentrated object, displaying a near-elliptical morphology. A discernible, albeit faint, disk-like structure appears to extend from the central bulge. The color profile suggests a dominant population of older stars, indicated by the redder hues in the outer regions, with a slightly bluer tint concentrated towards the nucleus, possibly indicative of some ongoing, albeit subdued, star formation activity within the core. There is no visible evidence of strong spiral arm structures, a prominent bar, or any major morphological disturbances indicating a recent major merger event. Minor asymmetries in the outer disk region suggest some level of gravitational interaction, although the source of this is not evident from this single image. Overall, it appears to be a lenticular-type galaxy, exhibiting characteristics intermediate between elliptical and spiral galaxies, possessing a generally smooth, rounded appearance with hints of disk-like features.
