The galaxy presents an overall elliptical morphology, appearing largely smooth and rounded in shape. There's a discernible central bulge that appears brighter and more concentrated. The color profile suggests a relatively evolved stellar population, dominated by older, redder stars in the bulge and a gradual shift toward slightly bluer hues in the outer regions, possibly indicating some ongoing, albeit modest, star formation. There is no obvious sign of spiral arms or a distinct disk structure, and there's no indication of a major ongoing merger event, though the galaxy appears somewhat disturbed, which could indicate a minor interaction in its past. The galaxy is of intermediate size, neither a dwarf nor an exceptionally large galaxy.
