The galaxy presents a predominantly smooth appearance, indicative of an elliptical morphology or a spiral galaxy viewed face-on at a significant distance where features are blurred. It appears largely spheroidal in shape, with minimal discernible spiral arm structure. There may be a slight asymmetry, although it is difficult to determine if this is due to an intrinsic feature or an artifact of the image. The color profile suggests a yellow-white central region, potentially indicating an older stellar population. There is subtle bluer emission extending outward from the central region, suggesting ongoing, but weak, star formation activity is taking place. The galaxy is moderately luminous, and it appears to be a relatively isolated object, showing no signs of major tidal disturbances or ongoing mergers with other galaxies in its immediate environment, however, there may be some minor disturbances, and it cannot be ruled out.
