The galaxy presents as a singular, relatively smooth object with a generally elliptical morphology. It exhibits a concentrated central region, potentially indicative of a galactic bulge. There is a noticeable color gradient, shifting from yellowish hues at the core to a slightly redder periphery, suggesting a differential distribution of stellar populations and/or dust content. The galaxy appears largely undisturbed with no obvious signs of tidal features, strong spiral arms, or active galactic nuclei based on visual inspection. It is consistent with a quiescent elliptical galaxy, potentially undergoing relatively low levels of star formation.
