The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a predominantly smooth and featureless morphology. Its overall shape is somewhat elongated, though largely rounded, lacking a clear spiral arm structure within the limits of image resolution. The central bulge is prominent, displaying a bright and concentrated luminosity. The color gradient appears to indicate that it is likely a population of older stars, with a small amount of ongoing star formation. There is no indication of strong tidal disturbances or a major merger event.
