The galaxy presents as a relatively compact structure, approximately 4 arcseconds in diameter, with a suggestion of disk-like morphology viewed at an angle. The central region is less defined than the galaxy's outer edges, with a smooth, diffuse appearance rather than a distinct bulge or nucleus. The color profile indicates a bluer hue, particularly at the center and extending outward, possibly indicating a presence of hot, young stars. The galaxy exhibits no obvious signs of a major ongoing merger, though there may be some minor irregularities or extensions suggesting past interactions. There is an absence of prominent spiral arms. Based on this information, the galaxy is likely a low mass spiral, or a blue compact dwarf galaxy.
