The galaxy presents a morphology characterized by a dominant, centrally concentrated luminosity. The core region appears smooth and spheroidal, exhibiting a yellowish-white color, indicative of an older stellar population. Extending outward from the core, a faint, diffuse disk is discernible, exhibiting some features and irregularities, some with what appears to be a more bluish-white tint, which suggest localized regions of active star formation. Faint hints of spiral arm structures are present, but the resolution is insufficient to resolve them distinctly. There is also the possibility of a minor interaction or merging event. The overall shape appears somewhat elongated, possibly indicative of tidal distortion.
