The galaxy presents as a largely smooth, elliptical structure. It exhibits a high degree of central concentration, with a gradual decrease in luminosity outward from the core. The galaxy appears nearly circular in projection, indicating a minimal inclination relative to our line of sight. There is no apparent dust lane or spiral arm structure visible. There appears to be only minor disturbances to its overall shape, which is generally consistent with a single galactic body. The color profile appears fairly uniform across the galaxy, exhibiting a yellowish-red hue, suggestive of an older stellar population.
