The galaxy presents a flattened, disk-like structure, suggesting it may be a spiral or lenticular type. A bright, concentrated central bulge dominates the core region, displaying a yellowish hue. The galaxy exhibits faint spiral arm-like structures extending from the central bulge, though these arms appear somewhat diffuse and lack well-defined boundaries. These spiral arm structures show blueish regions of what is assumed to be star forming regions. Overall, the galaxy's morphology appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The disk appears relatively smooth, but some faint disturbances and asymmetry can be noted.
