The galaxy presents a generally smooth morphology. It appears elongated, exhibiting a cigar-like shape. There is no distinct spiral structure or bar visible. The light distribution suggests a central bulge with a more diffuse halo extending outwards. Color gradients within the galaxy appear minimal, although the central region may be slightly bluer than the outer regions. There is no strong evidence of ongoing major mergers or significant tidal disturbances, although there may be minor asymmetries present. Overall, the galaxy appears relatively undisturbed. The light profile indicates a likely evolved system, with most of its star formation occurring at earlier epochs.
