The galaxy presents as a somewhat elliptical, though nearly circular, form. Its color profile suggests a dominant population of older stars, indicated by the yellowish-white hue concentrated towards the central bulge. There's evidence of a fainter, bluer disk surrounding the core, hinting at some ongoing, albeit subdued, star formation within the galaxy. The structure appears largely undisturbed, with no readily apparent signs of a major merger or significant tidal interactions. There may be some very minor disturbances present, such as a slight asymmetry or subtle irregularities in the outer regions of the galaxy. Overall, the galaxy appears relatively smooth and quiescent.
