The galaxy presents as a relatively smooth, elliptical structure. It has a concentrated, bright central bulge that dominates the overall luminosity. The light from the bulge appears yellowish-orange, suggesting a population of older stars. The outer regions exhibit a more diffuse and slightly bluer hue, potentially indicating the presence of some younger stars or ongoing, albeit limited, star formation. The overall shape is elongated, more akin to a flattened ellipse than a perfect sphere. There is no obvious evidence of spiral arms or significant dust lanes. The lack of major distortions implies the absence of recent major merger events, though some subtle irregularities in the outer envelope could hint at minor tidal interactions. The galaxy appears to be relatively isolated and well-defined, with no immediately obvious signs of a major ongoing interaction with another galaxy.
