The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color profile suggests a significant population of older stars, contributing to a yellowish-red hue. There is very little evidence of prominent spiral arms or significant dust lanes within the visible morphology. The galaxy appears to have a fairly regular, rounded shape. There's no immediately obvious sign of tidal disturbances, major mergers, or other significant gravitational interactions impacting the galaxy's overall structure. The light is concentrated at the core with a slow gradual decline towards the edges, and there is no evidence of active star formation.
