The galaxy presents as a disk-shaped system, viewed at a moderately high inclination. A prominent central bulge is observed, appearing relatively bright and concentrated. The disk component exhibits a somewhat clumpy and flocculent structure, hinting at ongoing or recent star formation activity. Dust lanes may be present, although not distinctly resolved, contributing to the irregular appearance of the disk. The galaxy appears to be somewhat elongated and not perfectly symmetrical, possibly indicative of interactions or internal asymmetries. Its color suggests a moderate population of young, hot stars, but also a significant presence of older stellar populations within the bulge. No obvious signs of a major merger are immediately apparent, though minor disturbances cannot be ruled out.
