The galaxy appears as a single, concentrated luminous object, likely an elliptical galaxy given its smooth morphology and lack of discernible spiral arms or a distinct disk structure. The light is concentrated in the center, with luminosity gradually decreasing outwards. It exhibits a yellow-red hue suggesting an older stellar population. The galaxy exhibits a somewhat circular morphology, although not perfectly round, it appears to be close to symmetric. There is a lack of any clear tidal features or significant asymmetries, indicating it is likely not undergoing a major merger currently, though it shows some signs of minor disturbances. Based on the color, the galaxy is likely not undergoing significant star formation.
