The galaxy presents as an elliptical morphology, with a smooth and concentrated light distribution. It exhibits a centrally dominant, bright core, suggesting a high concentration of stars or potentially an active galactic nucleus. The overall shape is moderately elongated. There is no visible evidence of spiral arms or prominent dust lanes. The color profile indicates an older stellar population, with a reddish-yellow hue most prominent in the central region, possibly indicating a dearth of ongoing star formation. No significant tidal features or distortions are apparent, suggesting it is not currently undergoing a major merger event, although there is potentially a minor disturbance. The galaxy is relatively compact in size, which is appropriate for its moderate mass, and displays a regular structure, with no obvious signs of significant recent starburst activity.
