The galaxy presents as a somewhat elongated, likely disk-shaped system, viewed at an oblique angle. The central bulge exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outwards from the bulge, a gradual color transition occurs towards the outer regions of the disk, where fainter, bluish patches are observed. These blue regions suggest the presence of younger, hotter stars and ongoing star formation. The overall morphology appears relatively undisturbed; there is no readily apparent indication of major merging activity or tidal disruption. It is likely a spiral galaxy but due to the viewing angle this cannot be said for certain. The galaxy is a very luminous object.
