The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, with a concentration of luminosity towards the center suggesting a possible bulge or nucleus. There may be some subtle disturbances in the light distribution of the galaxy, possibly indicating a minor interaction or internal structure. The overall color is bluish, suggestive of ongoing or recent star formation. There are no obvious spiral arms or a well-defined disk structure present, though an underlying disk cannot be ruled out. The galaxy is likely an elliptical or lenticular type with evidence of some recent star formation.
