The galaxy presents as an elongated, cigar-shaped object. It appears to have a smooth morphology with a slight central bulge. There is evidence of a disk-like structure that is somewhat disturbed, though there's no indication of a major ongoing merger or significant tidal features. The color profile suggests the presence of both older stellar populations and some active star formation, with bluer regions indicating areas of more recent star birth. The galaxy exhibits a relatively high luminosity, suggesting a substantial stellar mass.
