The galaxy presents as a relatively compact object, displaying a smooth, largely featureless morphology. A bright central region dominates, potentially indicative of an active galactic nucleus or a high concentration of stars. The overall shape appears to be generally rounded, with a slight extension suggesting a possible disk-like component. Color gradients are observed, with a bluer hue in the central core, which may indicate recent star formation, transitioning to redder colors in the outer regions, hinting at an older stellar population. No significant tidal features or signs of ongoing major mergers are immediately apparent, though subtle disturbances cannot be ruled out at this resolution.
