The galaxy appears to be a relatively smooth, early-type system, potentially an elliptical or lenticular galaxy. It exhibits a centrally concentrated luminosity profile, with the brightest region at the core gradually decreasing in intensity outwards. The morphology suggests a lack of significant spiral arm structure or prominent dust lanes. Its shape appears somewhat elongated but not strongly cigar-shaped, with the majority of classifications suggesting it falls between round and in-between. There is no readily apparent evidence of ongoing major mergers or significant tidal disturbances in the image. The galaxy exhibits a color gradient, transitioning from a yellowish or golden hue in the central region to a slightly bluer hue in the outer regions. The overall color suggests a stellar population dominated by older stars, with the possibility of some ongoing, but relatively low, star formation activity indicated by the outer region's bluer color.
