The galaxy presents a roughly elliptical morphology, exhibiting a relatively smooth light distribution, with indications of a central bulge. The galaxy's color profile suggests a mix of stellar populations; the central region appears yellower, possibly indicating older stars or dust extinction, while the surrounding areas appear bluer, potentially signifying the presence of younger, hotter stars. The presence of bluer regions hints at ongoing or recent star formation activity. There seems to be some interaction or distortion, but is hard to tell from the given image. The object exhibits signs of a substantial mass, inferred from its overall luminosity and the characteristics of its stellar population. The galaxy shows a degree of roundness.
