The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge that is notably yellow-orange in color, suggesting an older stellar population within the core. There is a slight elongation, with a mostly rounded morphology. The outer regions of the galaxy display a gradual fading in brightness and exhibit a somewhat bluer hue than the central bulge, which hints at the presence of younger stars within the galaxy's disk or outer halo. No strong tidal features or nearby companion galaxies are immediately apparent, implying that it is likely not undergoing a major merging event at this time.
