The galaxy presents as a single, relatively symmetric luminous object with a concentrated central bulge. The overall shape is generally round, without any apparent strong tidal features or morphological disturbances indicative of major mergers. The light profile appears smooth, lacking the distinct spiral arm structures or prominent dust lanes often associated with disk galaxies. The core of the galaxy is bright, suggesting a high concentration of stars, potentially an actively star-forming region or an active galactic nucleus. There's a faint, diffuse halo or extended envelope surrounding the central region, indicating the presence of older stellar populations extending beyond the main body of the galaxy. The color gradients within the galaxy are subtle, with a slightly bluer hue in the outer regions and a warmer tone towards the core.