The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears somewhat spherical in shape. There is no obvious disk structure or prominent spiral arms visible. The core of the galaxy is bright, suggesting a higher concentration of stars or a possible active galactic nucleus. The galaxy's color profile indicates a mature stellar population, potentially with limited ongoing star formation. No significant tidal distortions, merger features, or dust lanes are readily apparent within the galaxy's structure. There might be slight disturbances, but it is generally an isolated galaxy. The galaxy displays a notable halo, exhibiting a gradual decrease in luminosity from the core outwards.