The object presents as a slightly elongated, diffuse structure with a relatively low surface brightness. It is predominantly blue in color, suggesting the presence of a younger stellar population. The overall morphology is irregular, lacking a distinct spiral arm structure or a well-defined elliptical shape. There appears to be a slight asymmetry to the object. Patches of varying intensity are observable throughout the galaxy, potentially indicating differing densities of stars or gas. There is evidence of minor disturbances in the galaxy's shape, which may suggest a past or ongoing interaction with another galaxy. These disturbances may also indicate the presence of internal dynamic processes causing irregularities in the structure. There is no evidence of a prominent central bulge, and no tightly wound spiral arms. 
