The galaxy presents as a single, relatively smooth light distribution. Its morphology is generally elliptical, exhibiting a high degree of circularity. A pronounced central bulge dominates the galaxy's structure, displaying a bright, concentrated luminosity. The color profile suggests an older stellar population in the bulge. The outer regions are less luminous and appear bluer, potentially indicating the presence of younger stars or ongoing star formation, though at a low rate. There are no visible tidal features or strong asymmetries, suggesting it has not undergone recent major mergers or significant gravitational interactions. The overall structure is indicative of a galaxy that has largely completed its evolutionary process, trending toward a more quiescent state.
