The galaxy exhibits a generally smooth morphology, although there appears to be some degree of disturbance in its structure. It is somewhat elliptical in shape, tending towards an intermediate classification between round and elongated. There's a noticeable central bulge that is bright and concentrated, likely indicating a significant population of older stars. The overall color suggests a mix of stellar populations, with a blueish hue in the outer regions implying ongoing star formation. Faint, extended features appear to disrupt the smoothness, potentially suggesting interactions or minor mergers in its past or present. The central region appears dominant, obscuring a clear view of a potential disk.
