The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, appearing yellow-white. The galaxy's light gradually fades outward from the center, exhibiting an intermediate ellipticity, close to a rounded shape. There is a faint suggestion of a disk-like structure. No prominent spiral arms are visible, nor are there indications of significant dust lanes. Close inspection reveals no obvious signs of tidal disturbances or ongoing major mergers, though a subtle asymmetry may imply minor gravitational interaction. Based on the color profile, the stellar population is primarily composed of older stars, and star formation activity appears to be low.
