The galaxy appears as a centrally concentrated object with a smooth morphology. Its overall shape appears somewhat elongated but largely spheroidal, hinting at a possible elliptical or S0 classification. The central region exhibits a brighter, more intense luminosity. There is evidence of some disruption, with the outer regions exhibiting a faint, diffuse halo extending asymmetrically from the main body. This could be evidence of a minor interaction with another galaxy or tidal stripping. The light profile suggests a relatively old stellar population, though there's a hint of bluer light in the outer regions, which may indicate recent or ongoing star formation activity. Overall, this galaxy seems to be at a stage of transition, possibly evolving from a more active spiral galaxy towards a quiescent elliptical.
