The galaxy presents as a spiral type with a generally ordered morphology. It exhibits a discernible disk structure that is viewed at a moderate inclination, showing some obscuration. The galaxy's nucleus appears bright and concentrated, suggesting a substantial central bulge component. Spiral arms are present and relatively well-defined, emanating from the central bulge, and loosely wound. The arms exhibit some degree of patchiness, possibly indicative of active star formation regions. The color distribution reveals a yellowish hue in the central bulge, transitioning to a bluer tint in the outer spiral arms. No signs of major merging activity are readily apparent, though some minor asymmetries in the outer disk could suggest past interactions or ongoing accretion events. A faint bar seems to cross the galaxy's bulge.