The galaxy presents as a relatively compact object. Its core region exhibits a bright, concentrated luminosity, suggestive of either an active galactic nucleus or a dense stellar population. The overall morphology appears somewhat disturbed, potentially indicating ongoing or recent interactions. There are possible minor disturbances detectable. Faint emission suggests the presence of a weak, distorted disk structure. There is also some evidence of what might be a faint tidal tail emanating from the main galactic body, potentially a result of a past minor merger event. The light from the galaxy is most intense in blue, followed by green then red.
