The galaxy presents a smooth, elliptical morphology. The central region exhibits a bright, concentrated bulge, characterized by a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the luminosity decreases gradually, forming a diffuse halo. There is little evidence of spiral arms or prominent dust lanes, and it appears relatively undisturbed, with no signs of significant tidal distortions or interactions. The overall shape is somewhat elongated, but not extremely so. The faint outer regions suggest a more extended structure, though the image resolution limits detailed analysis of its morphology. Star formation appears to be low, inferred from the color and lack of obvious HII regions. The galaxy's structure seems consistent with an early-type galaxy.
