The galaxy appears to be an elliptical type. It has a smooth, largely featureless morphology, with no apparent spiral arms or significant dust lanes. The light distribution appears concentrated towards the center, with a gradual decrease in brightness as one moves outward. The core region exhibits a yellow-white hue, suggesting a population of older stars. Fainter, diffuse light surrounds the core, extending along what appears to be a major axis. The galaxy shows signs of potential interactions with other galaxies. There are some disturbances in the shape of the galaxy, potentially from an ongoing merger event with a smaller galaxy, or a tidal disruption. The overall color is consistent with an older stellar population and a relatively low rate of current star formation. 
