The galaxy appears to be a relatively compact object with a centrally concentrated luminosity profile. Its morphology is predominantly smooth in nature, lacking any obvious spiral arms or distinct features. The shape is largely amorphous with slight ellipticity, appearing neither perfectly spherical nor highly elongated. There is a hint of subtle disturbance or asymmetry in its outer regions, however, this is not indicative of a major merger event. The galaxy's color index suggests moderate star formation activity, which is plausible if it is a relatively undisturbed system with an old stellar population. A possible minor disturbance is present, but is difficult to assess.
