The galaxy presents as a relatively compact object with an estimated effective radius of approximately 7 arcseconds. It exhibits a centrally concentrated light profile, suggesting the presence of a bulge component. The overall color appears predominantly blue, indicative of ongoing star formation and a relatively young stellar population. There is a subtle disk-like structure observed, however, it's morphology is not clearly defined. There appear to be minor disturbances within the disk region, which may be indicative of a small merging event or recent gravitational interaction. A small plume, redder in color, is present in the upper region, possibly indicating a tidal tail or an area of dust obscuration.
