The galaxy presents as a relatively smooth, elliptical-shaped object with a noticeable central bulge. It exhibits a yellowish core, likely indicative of an older stellar population. Moving outward from the core, the galaxy transitions to a bluer hue in its outer regions, suggesting the presence of some younger stars or ongoing star formation, albeit at a lower rate. The overall structure appears undisturbed, without any prominent spiral arms or tidal features. The light distribution suggests a gradual decrease in stellar density from the center outwards. The ratio of the semi-major to semi-minor axis implies a moderately flattened shape, though it's not significantly elongated.
