The galaxy presents a somewhat elliptical morphology, with a smooth, centrally concentrated bulge that appears yellow to golden in color. Surrounding the central bulge, there is a fainter, more diffuse disk component, exhibiting a bluish hue. This suggests the presence of a younger stellar population within the disk, possibly indicative of ongoing or recent star formation. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers. There is a slight elongation, but not significant enough to classify it as a highly barred spiral or irregular galaxy. The light appears to be more focused in the central area, with light decreasing as it radiates outwards.