The galaxy presents a complex morphology, appearing as a disturbed disk galaxy. While a distinct bulge component is not readily apparent, the central region is characterized by a bright, concentrated area of light. Faint spiral arms may exist, though their structure is somewhat disrupted, potentially indicating gravitational interactions. There is also a tidal tail emanating from the galaxy, indicating a possible merger. Overall it is an intermediate mass galaxy, likely with a moderate rate of star formation.
