The galaxy exhibits a somewhat disturbed morphology, potentially indicative of a past or ongoing interaction with another galaxy. There is a significant central bulge with a yellowish hue, suggesting an older stellar population dominating the core. Extending from the central region, there's evidence of more diffuse, fainter spiral arms, which appear somewhat disrupted, with one arm appearing significantly less defined. These arms show hints of blue, implying the presence of younger, hotter stars and regions of active star formation. There is a region above the nucleus that shows a distinct red clump. Overall, the galaxy appears to be undergoing a transition, with a central concentration of older stars but with a notable level of ongoing star formation in the extended disk.
