This galaxy presents as a relatively smooth, elliptical morphology. It exhibits a central bulge that appears to be brighter and more concentrated, gradually fading into a diffuse outer halo. The galaxy has a slightly elongated shape, appearing somewhat cigar-shaped rather than perfectly round. There are no obvious signs of significant spiral arm structures or prominent dust lanes. The overall color of the galaxy leans toward a bluish-white hue, suggesting the presence of a population of relatively young, hot stars, although star formation rates are likely low. There are subtle indications of minor disturbances in its overall structure which might suggest past gravitational interactions, but this galaxy is generally not undergoing any major merging events or violent disruptions.
