The galaxy presents as a somewhat elliptical structure with a smooth, diffuse appearance. A concentrated, bright central bulge of older stars is apparent, with a more diffuse halo extending outwards. The color profile suggests a galaxy population dominated by older stars, exhibiting a yellowish hue, with possible hints of bluer regions on the outer edges, indicating ongoing, but limited, star formation. The overall structure suggests a lack of significant recent major mergers, though minor tidal disturbances cannot be ruled out based on the image alone.
