The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellowish hue, possibly indicating an older stellar population. Surrounding the central bulge, a more diffuse and bluer halo extends outwards, suggesting the presence of a younger stellar population and/or ongoing star formation activity. The galaxy appears largely undisturbed, with no obvious signs of major merging events or tidal disruptions. There are hints of subtle irregularities or faint features within the outer halo. The overall morphology is largely smooth, but there may be faint, subtle structures present within the galaxy.
