The galaxy presents as a relatively smooth, elliptical-like structure, possibly an early-type galaxy. Its overall shape is elongated. The light distribution is centrally concentrated with a gradual decline in brightness towards the outer edges, indicating a lack of distinct spiral arms or features typically associated with disk galaxies. The central region exhibits a yellowish or reddish hue suggesting an older stellar population. The galaxy appears relatively isolated, displaying no obvious signs of ongoing major mergers or significant tidal interactions with other galaxies. Some disturbances seem to be present in its shape, potentially a minor interaction. It presents a high mass and moderate star formation. Overall, the galaxy appears as a well-evolved system dominated by an older population of stars, consistent with a passive evolutionary state.
