The object appears to be a relatively smooth galaxy with a generally elliptical morphology. The galaxy exhibits a bright central bulge or core, surrounded by a more diffuse halo. A slight hint of a disk or spiral arm structure may be present, but it is not distinctly defined. The galaxy’s color suggests a population of older stars, with a subtle blueish tint in some regions indicating the presence of some younger, hotter stars. The galaxy is overall relatively isolated. There might be some indication of a minor interaction or disturbance, but the galaxy’s structure appears largely undisturbed, and does not show any obvious evidence of ongoing or recent major mergers. The shape of the galaxy appears mostly round.
