The galaxy appears to be a relatively smooth, elliptical system, with a slight elongation. The central region is characterized by a bright, concentrated luminosity, suggestive of a dense stellar population and potentially a supermassive black hole. The overall color is yellowish, indicating an older stellar population and a relatively low rate of ongoing star formation. There is some indication of a faint disk structure but the disk is not well-defined and has no visible spiral arms. There are no signs of major disturbances or mergers, suggesting it's a relatively isolated and dynamically stable system. Overall, it appears to be an early-type galaxy, potentially an elliptical or lenticular type, at a considerable distance.
