The galaxy appears to be a relatively compact object with a bright, concentrated core region. The overall shape is somewhat irregular, lacking a well-defined spiral structure. The color profile suggests the presence of both younger, bluer stellar populations, concentrated primarily towards the galaxy's core, and older, redder populations in the outer regions. There is potential evidence of some minor disturbances or tidal features, visible as slight asymmetries in the outer halo region. The data suggests that the galaxy is not currently undergoing a major merger event, although subtle interactions or minor mergers cannot be ruled out.
