The galaxy presents as a largely featureless, elliptical morphology. It appears to be highly concentrated, with a smooth, diffuse light profile. The core of the galaxy exhibits a yellow-orange hue, suggesting an older stellar population dominating the central regions. Fainter greenish color surrounding the core indicates the presence of some younger stars, but overall star formation is generally low. The galaxy exhibits a nearly circular shape. There is no visual evidence of significant tidal disturbances or ongoing mergers; it appears to be an isolated system with a well-defined structure.
