The galaxy presents a generally smooth and rounded morphology. It exhibits a bright central bulge that graduates into a fainter, diffuse halo. The light distribution suggests a lack of prominent spiral arms or other distinct features. There are slight color variations within the halo, with hints of reddish hues toward the outer regions possibly indicative of an older stellar population, and some slightly bluish tints closer to the center, potentially suggesting a more active star forming region. There is no apparent evidence of major mergers or tidal disturbances within the galaxy's structure.
