The galaxy presents a somewhat smooth, elongated morphology. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. The light distribution fades gradually from the core outwards, implying a lack of strong spiral arm features. The overall shape appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions, though a very slight asymmetry may be present. The overall color gradient suggests some ongoing, albeit subdued, star formation activity, primarily in the outer regions, implied by a faint bluish tint.
