The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core, suggestive of a significant stellar bulge. There is no discernible spiral arm structure or distinct disk component visible at this resolution. The overall color appears relatively red, indicating a population of older stars and a relatively low rate of ongoing star formation. There might be minor irregularities or disturbances in the outer regions, but the galaxy's overall structure is generally undisturbed. The galaxy appears to be a fairly massive system.
