The galaxy presents as a moderately bright, relatively compact object. Its overall morphology appears smooth and elliptical, lacking any prominent spiral arm structures or a distinct disk. There is a slight elongation to its shape, appearing more "in between" rounded and cigar shaped. The galaxy's core exhibits a concentrated central bulge, appearing somewhat yellow. This suggests a higher density of older stars. The outer regions of the galaxy exhibit a more gradual decrease in brightness, with a smooth transition outwards. There are no readily apparent signs of ongoing major mergers or tidal disturbances, suggesting a relatively settled state. Possible minor disturbance in morphology. Color gradients suggest variations in stellar populations. Overall, the galaxy appears as a well-evolved, quiescent system with minimal current star formation.
