The galaxy appears as a centrally concentrated elliptical system, exhibiting a smooth, featureless morphology. The core displays a bright, relatively uniform emission profile, indicative of an older stellar population. The overall shape is slightly elongated, exhibiting a mild ellipticity. The galaxy is approximately 3.2 kpc in radius. The color profile appears somewhat redder. There is no visible evidence of ongoing star formation regions or spiral arm structures, suggesting a lack of significant recent mergers or interactions.
