The galaxy presents as a moderately inclined disk, appearing somewhat elliptical in shape with a cigar-like form. The central region exhibits a bright, concentrated bulge with a yellowish-white hue, suggesting a substantial population of older stars. Moving outward from the bulge, the galaxy transitions to a fainter, bluer color, indicative of younger stars and potentially ongoing star formation within the disk. The disk itself appears relatively smooth and lacks distinct spiral arm structures. The overall light distribution indicates a relatively well-defined structure without obvious signs of major disturbances or merging events. The galaxy appears to be a relatively isolated system without nearby companions strongly influencing its morphology.
