The galaxy presents as a spiral type, exhibiting well-defined, loosely wound spiral arms. It has a moderate-sized bulge, and the disk is oriented at an angle relative to our line of sight. There is evidence of an interaction or possible merger event, visible as a significant disturbance in the galaxy's morphology. The spiral structure appears asymmetric, with one side exhibiting more pronounced disruption than the other. There may be a faint bar structure bisecting the bulge, though this is not definitively discernable. Star formation appears to be present, indicated by bluer regions within the spiral arms, as well as a redder clump that could represent a region of more dust-obscured star formation. The overall color suggests a mature stellar population in addition to the star-forming regions.
