The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The core appears more luminous and exhibits a slightly redder color index than the overall halo. There is only a hint of possible spiral structure. The galaxy does not display any prominent dust lanes, tidal tails, or other indications of a major recent merger event. The overall shape appears somewhat rounded, not excessively elongated or cigar-shaped. The galaxy may be undergoing little to no star formation currently.
