The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge dominates the overall structure, exhibiting a yellowish-white hue indicative of an older stellar population. Surrounding the central bulge, a fainter, more diffuse halo is observed. Faint bluish tinges are present in the outer regions of the halo, suggesting the presence of some younger, hotter stars or ongoing star formation, though this activity appears subdued. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears relatively undisturbed, showing no signs of major merger events or tidal disruptions. Its shape is more in between elliptical and round, but it is closer to round.
