The galaxy presents as a single, concentrated object with a smooth, largely featureless morphology. The central region exhibits a bright, relatively homogenous luminosity profile, suggesting a high concentration of stars and potentially a central supermassive black hole. The galaxy appears roughly circular, with a slight extension that may indicate a mild departure from perfect sphericity or the presence of a weak tidal interaction. Color gradients are subtle, with a possible trend towards redder hues in the central region and bluer shades toward the outer edges, which could reflect differences in stellar populations or dust distribution. There is no evidence of spiral arms, a bar structure, or significant dust lanes. Overall, the galaxy appears to be a relatively relaxed system.
