The galaxy presents as a largely featureless, elliptical-like structure with a high degree of central concentration. The light distribution is smooth and diffuse, showing no obvious spiral arms, bars, or prominent dust lanes. The core region appears brighter and slightly more yellow than the outer regions, which fade gradually into the background sky. There is a hint of blue-green tint toward one edge of the central region, suggesting a minor presence of younger stars or active star formation. Overall, the galaxy's morphology is indicative of an evolved system dominated by an older stellar population. There may be some minor disturbance in the form of asymmetry.
