The observed galaxy presents as an apparent disk galaxy, viewed at a high inclination angle. Its structure is primarily composed of a central bulge region that displays a strong concentration of light, exhibiting a yellowish-white hue, which could imply an older stellar population. Extending outward from the bulge, a flattened disk structure can be discerned; however, the high inclination makes it difficult to resolve spiral arm details. The disk appears asymmetric. The disk's color gradients suggest a potential mix of stellar populations, with a slightly bluer component possibly indicating ongoing star formation. Evidence of possible minor disturbances and asymmetries in the disk morphology could be related to interactions with companions. The overall morphology also hints at a possible merger event.
