The galaxy presents as a relatively smooth, elongated structure. It displays a central bulge that exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy show a bluish tint, potentially indicating areas of more recent star formation. The overall shape is somewhat cigar-like. There are no readily apparent spiral arm structures or strong dust lane features visible in this image. It appears relatively undisturbed, with no major signs of an ongoing merger. However, some minor disturbances cannot be ruled out at this resolution.
