The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It exhibits a noticeable elongation, appearing more cigar-shaped than circular. There is no clear evidence of spiral arm structure or distinct disk features. The light profile suggests a dominant bulge or spheroidal component. Faint extensions or tidal features may be present but are not definitively discernible given the image quality. There is no indication of a major ongoing merger, though the possibility of minor disturbances or past interactions cannot be ruled out. The galaxy displays a relatively blue hue, which could indicate ongoing star formation, although the smooth morphology is typically associated with older stellar populations.
