The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. It appears moderately flattened. The luminosity profile increases sharply toward the center, suggesting a high stellar density in the core. There is some indication of an extended halo of fainter, diffuse light surrounding the main body, though it is not sharply defined. The galaxy has a slightly elongated shape, and shows little evidence of spiral arms or significant dust lanes. Color gradients are subtle, with the central bulge appearing slightly yellower than the outer regions. There does not appear to be a substantial amount of active star formation within the galaxy. The morphology suggests an evolved system, likely dominated by an older stellar population. There are no obvious signs of ongoing mergers or tidal disturbances.
