The galaxy presents as a disk-like structure, viewed at a slight angle. The central region exhibits a higher concentration of light, suggestive of a bulge component. This bulge appears yellowish-white, indicative of an older stellar population. Extending outwards from the central region, the disk displays a less uniform color distribution with patches of blue. These blue areas are likely regions of active star formation. A faint tail or arm-like structure is noted in the upper region of the galaxy, displaying the same blue color of active star formation. Overall, the galaxy's morphology leans towards a spiral or barred spiral type, although the resolution limits a definitive classification. The overall shape appears relatively undisturbed, with only minor asymmetrical features.
