The galaxy presents a generally smooth morphology, with a centrally concentrated light profile. There is little evidence of spiral arm structure or prominent dust lanes. The overall shape is relatively round, displaying a slight ellipticity. Color gradients suggest a possible redder core region, with a gradual shift toward slightly bluer hues in the outer regions, indicating potentially younger stellar populations. The system does not appear to be undergoing any major merger activity or exhibiting strong tidal features, although very minor distortions could potentially be present at the limits of resolution.
