The galaxy presents as a moderately bright, elliptical object with a high degree of central concentration. The core is a luminous, yellowish-white, suggesting a significant population of older stars. Moving outward from the core, the light gradually diminishes, transitioning into a less defined, reddish-hued halo. The overall shape is slightly elongated. There is no apparent spiral structure, nor are there any significant dust lanes or prominent star-forming regions visible. The smooth appearance suggests a relatively evolved system with little ongoing star formation. The galaxy's color indices indicate a relatively red population, consistent with an older stellar population.
