The galaxy presents a primarily smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's overall structure, with a gradual decrease in surface brightness moving outwards. The core exhibits a yellowish hue, possibly indicating a population of older stars. Fainter, bluer regions appear sporadically in the outer halo. These regions might be indicative of pockets of more recent star formation, although they contribute a small fraction to the overall light. There is no obvious presence of spiral arms or a prominent disk. The galaxy appears relatively isolated, displaying only slight irregularities in shape.
