This galaxy exhibits a complex morphology, appearing somewhat elongated and disturbed. A central, brighter region is apparent, suggesting a concentration of older stars and possibly a bulge component. This central area exhibits a yellow hue. One end of the galaxy shows a distinct, reddish-orange patch, which may indicate a region of active star formation or dust obscuration. Fainter, bluer light extends from the galaxy, possibly indicating a disk or spiral arms, or recent or ongoing star formation. The overall structure suggests that the galaxy may be undergoing a minor interaction or have experienced one in the past, as indicated by its disturbed shape.
