The galaxy presents as a moderately luminous, elongated structure, indicative of a disk galaxy viewed at an oblique angle. A prominent central bulge is apparent, displaying a yellowish-orange hue that suggests a population of older stars. Moving outwards from the bulge, the disk shows a bluer tint. Faint indications of spiral arm structures are present but not sharply defined. There may be a bit of ongoing star formation, primarily in the outer regions, judging by the bluer color. The galaxy's outer edges fade gradually into the background, suggesting a diffuse stellar halo. There is no obvious tidal features or strong indications of recent major mergers.
