The galaxy presents as an elliptical type, elongated in shape, exhibiting a smooth, featureless morphology. The central bulge appears bright and concentrated, displaying a yellowish hue indicative of an older stellar population. Surrounding the core, a diffuse, bluish halo is observed, likely representing a region of more recent, albeit subdued, star formation activity. The overall structure suggests a system undergoing a relatively quiescent phase in its evolution, with minimal signs of ongoing mergers or significant tidal disturbances. The galaxy's orientation provides a near edge-on view, enhancing the perceived ellipticity.
