The galaxy appears as a lenticular or possibly an elliptical galaxy, exhibiting a smooth, featureless morphology in this observation. It possesses a central bulge that is significantly brighter than the outer regions, suggesting a high concentration of stars in the galactic nucleus. The light distribution shows a gradual decrease in intensity from the core outwards, forming an elongated shape, indicating a notable ellipticity. The color indices suggest a population of older stars, resulting in a reddish hue within the galaxy. There is no visual evidence of active star formation regions or prominent spiral arms. Overall, this galaxy exhibits characteristics consistent with an evolved stellar population and a relatively quiescent state in terms of star formation activity.
