The galaxy presents a generally smooth and elliptical morphology, exhibiting a moderate ellipticity. The central region is characterized by a bright, concentrated nucleus, suggesting a high stellar density. Progressing outwards from the nucleus, the luminosity gradually decreases, displaying a diffuse and extended halo structure.

There is a subtle color gradient across the galaxy. The central bulge appears more yellow, likely indicating an older stellar population, while the outer regions exhibit a slightly bluer hue, hinting at the presence of younger stars or ongoing star formation, albeit at a relatively low rate.

There is no prominent evidence of distinct spiral arms or strong dust lanes. The overall structure appears relatively undisturbed, without significant signs of tidal interactions or recent mergers.
