This galaxy appears to be a relatively smooth and centrally concentrated system. It exhibits a generally elliptical morphology, with the major axis slightly elongated. There is a bright core, indicative of a high density of stars or potentially an active galactic nucleus, surrounded by a more diffuse halo. The color profile is bluer in the outer regions, suggesting ongoing star formation or a younger stellar population compared to the redder, older stellar populations in the central bulge. There may be some subtle features indicative of minor disturbances, but overall the galaxy appears relatively undisturbed, without strong evidence of a major merger event. The galaxy's estimated size would make it a typical galaxy. The overall characteristics align with a moderate-mass galaxy with ongoing, but not exceptionally high, star formation activity.
