The galaxy presents as a generally elliptical morphology, exhibiting a smooth appearance with a prominent central bulge. It has a cigar-like shape with a ratio greater than 3:1 between its major and minor axes. The color profile suggests a greater concentration of older stellar populations, indicated by the yellowish-red hue of the bulge and surrounding halo. There may be hints of some disk-like features but the galaxy appears to be mostly spheroidal. There is no obvious evidence of recent or ongoing major mergers or tidal disturbances; the galaxy exhibits a largely undisturbed form.
