The galaxy exhibits a flattened, elongated morphology, appearing cigar-shaped in projection. Its light profile suggests a relatively smooth distribution of stars, though there is some evidence of disk-like structure. The central region is dominated by an orange-yellow hue, indicative of an older stellar population. Fainter blueish light is distributed in the surrounding area, suggesting recent or ongoing star formation. There appears to be some minor disturbances in the arm structure, possibly due to a minor merger.
