This galaxy appears to be relatively small in angular size, covering an estimated area suggesting a compact morphology. The galaxy exhibits a dominant central bulge. Within this central region, there is a strong concentration of light, indicating a high stellar density. The overall color is complex, with the central regions appearing predominantly redder, potentially indicating an older stellar population or significant dust obscuration. There are possible faint, irregular features extending outward from the central region. Based on the disturbance, the possibility of an ongoing or recent merger cannot be ruled out. The features are faint, and difficult to resolve given the seeing conditions. Additional data, such as spectroscopic redshift information, would be needed to confirm the true nature and distance of the object.
