The galaxy presents as an elongated, disk-like structure, with a noticeable bulge at its center. The central region exhibits a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the disk appears to have a spiral arm structure, which is slightly disrupted on one side. This disruption is evidenced by an irregular, reddish area, potentially indicating ongoing star formation or interaction with a smaller companion. The spiral arms show some bluer regions intermixed with yellower tones, consistent with the presence of younger, hotter stars alongside older stellar populations. Overall, the galaxy appears to be undergoing some form of interaction or disturbance, but maintains a generally well-defined, disk-dominated morphology.
