The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The central bulge exhibits a high surface brightness and a yellowish-white color, suggesting an older stellar population. Moving outward from the core, the color transitions to a slightly redder hue, indicating possible variations in stellar age or dust content. The overall shape is approximately round, with minimal evidence of spiral arms or a distinct disk structure. There is a slight elongation but it appears to be somewhat spherical in nature. The outer edges of the galaxy fade gradually into the background sky, which suggests the galaxy is likely an elliptical. No signs of major mergers or significant tidal disturbances are readily apparent from the image.
