The galaxy appears as a moderately bright, compact object with a diffuse, somewhat irregular morphology. The core region exhibits a slightly elongated structure, possibly indicative of a disk or bar. There is evidence of some disturbed features or faint tidal tails extending outwards, suggesting past or ongoing interactions or mergers. A few brighter knots of emission are observed within the galaxy, likely regions of active star formation. Overall, the galaxy appears to be in a state of transition, potentially evolving through mergers, starbursts, or AGN activity. Its general color suggests an intermediate stellar population with ongoing star formation.
