The galaxy presents as a somewhat smooth, disk-like structure with a central bulge. The core exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. Moving outwards from the core, the overall color shifts towards a bluer hue, particularly along what appears to be the edges of the galactic disk. This suggests the presence of younger, hotter stars and regions of on-going star formation. There is no strong indication of spiral arm structure. The disk exhibits a slight degree of asymmetry, potentially indicating a minor gravitational disturbance or tidal interaction. The galaxy does not appear to be undergoing a major merging event.
