This galaxy appears to be a spiral type, although the resolution limits detailed morphological classification. The galaxy exhibits a prominent central bulge. Two distinct spiral arms emerge from the nuclear region, tracing an ordered pattern. The arms are relatively tightly wound. A bar structure is present across the central region. There may be weak evidence of dust lanes within the disk, contributing to the observed color variation. The bulge is elongated. There is no evidence of any interaction or merging activity.
