The galaxy presents as a diffuse, somewhat amorphous structure. It exhibits a faint, elongated form without a well-defined nucleus or distinct spiral arm morphology. There is a subtle hint of a disk-like structure; however, the galaxy appears dominated by a smooth distribution of light. The color distribution suggests a relatively even population of older stars, possibly indicating an elliptical galaxy. The low surface brightness suggests a significant distance or a population of intrinsically faint stars. There appears to be minor disturbance as there may be a faint tidal tail present. More information is needed.
