The galaxy presents as a relatively smooth, disk-like structure with a prominent central bulge. It is oriented with its major axis roughly horizontal. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. A diffuse disk surrounds the bulge, appearing more bluish-white, potentially indicating regions of more recent or ongoing star formation. Overall the galaxy appears to be relatively undisturbed with no obvious signs of spiral arms, merging events, or significant tidal features. The elongation is moderate; it is neither perfectly circular nor highly flattened. 
