The galaxy presents a generally smooth, elliptical appearance. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color gradient indicates a yellowish hue in the central area, potentially suggesting an older stellar population. A hint of reddish hue may indicate the presence of dust in the outer reaches. Overall, there is no definitive evidence of significant disk structure or spiral arms. No major mergers or interactions with other galaxies are apparent, though a minor irregularity is observed on the lower left of the galaxy.
