The galaxy presents as a smooth, elongated structure. It displays a somewhat cigar-shaped morphology. There is a central bulge or core that exhibits a more concentrated, brighter luminosity, with color appearing more yellow. Fainter, bluer hues are observed in the outer regions of the galaxy, indicating some star formation. The galaxy lacks any obvious spiral arm structures or prominent dust lanes; it seems to be a relatively homogenous distribution of stars. There is no sign of any tidal tails or major disturbances indicative of a recent major merger. There is a slight hint of a disk shape, but the bulge seems to be dominating the galaxy's morphology.
