The galaxy presents an apparent elliptical morphology, although some irregular features are present. The central region displays a high concentration of light, appearing bright white. A subtle disk-like structure may be present, but it is not sharply defined. A distinct blue-ish region is visible on one side of the galaxy, possibly indicating an area of recent star formation. Overall, there is evidence of some gravitational disturbance or interaction, potentially due to a past or ongoing merger. The galaxy appears to be a relatively low-mass system with a low star-formation rate.
