The galaxy appears as a generally smooth structure, with a slightly elongated shape. The central region exhibits a higher surface brightness, suggesting a concentration of stellar mass and/or an active galactic nucleus. The light distribution is not perfectly circular, showing some deviation towards an intermediate ellipticity. There is a hint of asymmetry, possibly indicating minor disturbances in the galaxy's morphology. The overall color suggests a population of relatively old stars, with a slight bluer tint in the outer regions, potentially indicating recent star formation, although at a low rate. There does not appear to be an obvious spiral arm structure or prominent dust lanes. There is no evidence of any major ongoing mergers, although the slight morphological disturbances may suggest past interactions. The galaxy appears to be relatively isolated within its immediate environment.
