The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. It exhibits a somewhat flattened disk-like structure extending outwards from the core region. The overall color profile indicates a population of older stars, with a gradual color shift from slightly bluer regions in the outer disk to a redder hue in the central bulge. There are some indications of minor disturbances or irregularities in the galaxy's structure, possibly hinting at past or ongoing interactions. It is likely a galaxy with an estimated stellar mass of 10^10 solar masses, with low to moderate ongoing star formation activity. 
