The galaxy appears to be a spiral galaxy, though it has some distinguishing features. A prominent central bulge is noticeable, exhibiting a yellowish-white hue, suggesting an older stellar population. The spiral arms are somewhat diffuse and not sharply defined, with some indications of bluer regions, potentially indicative of ongoing star formation. One side of the galaxy appears to be more heavily disturbed than the other, showing signs of tidal disruption or possible interactions with a smaller companion. Overall, the galaxy presents a complex morphology, showing characteristics of both mature and active processes.
