The galaxy presents as a spiral with a moderately sized bulge. The spiral arms are quite distinct and well-defined, exhibiting a relatively open structure. There is no strong bar feature visibly present. The color gradient indicates ongoing star formation, particularly within the spiral arms which appear bluer than the central bulge. There is evidence of some disturbance within the structure, but not a major merger event. It appears to be in the process of merging with a nearby galaxy and has a high likelihood of having spiral arms.
