The galaxy presents a generally smooth morphology, characterized by a centrally concentrated bulge. The light distribution appears roughly circular, with some indication of ellipticity, though the overall form is largely spheroidal. 

The central region is bright and shows a cyan color, possibly indicating active star formation. Fainter light extends outward from the central core. The colors seem to shift outwards from blue to more reddish hues. 

There is no clear evidence of spiral arm structure or a well-defined disk. A faint asymmetry is noticeable in the outer regions, potentially suggesting minor gravitational interactions or internal disturbances. Overall, the galaxy appears to be relatively undisturbed, without strong tidal features or indications of a major ongoing merger.
