The galaxy presents a generally smooth morphology, suggesting an elliptical classification. The central region exhibits a bright, concentrated bulge, appearing yellowish-orange, which may indicate an older stellar population dominating the core. Moving outwards, there is a gradual decrease in luminosity. Faint, diffuse bluish regions can be observed in the outer areas of the galaxy, possibly indicating pockets of younger, hotter stars, though their contribution to the overall color is minimal. There is no discernible spiral arm structure or any apparent major disturbances. The galaxy appears somewhat elongated, but is closer to a circular shape. Faint signs of minor tidal disturbances may be present, but are not obvious.
