This galaxy presents a generally smooth appearance, with a notable concentration of light toward the central region. The galaxy exhibits an elliptical shape, appearing somewhat elongated. There is a distinct color gradient visible, shifting from a bluer hue in the outer regions to a more yellowish/reddish hue towards the center. This may indicate a higher proportion of older stars in the central bulge compared to the disk. There is a hint of some minor disturbances to its structure, indicating it may have had a past interaction. It is likely undergoing star formation at a low to moderate rate. Overall, this galaxy is a relatively massive and well-evolved system, with hints of past interactions.
