The galaxy appears as a centrally concentrated, elliptical system. The core exhibits a bright, relatively smooth morphology, with a gradual decrease in luminosity extending outwards. There is some evidence of a disk structure, it is not very clear. The galaxy's color profile suggests a dominant older stellar population. Based on the tidal disturbances, this system shows signs of an ongoing or past minor merger event. The lack of significant dust lanes or prominent spiral arms further supports the classification of this object as an early-type galaxy, potentially an elliptical galaxy undergoing minor interactions.
