The galaxy presents a smooth, elliptical morphology, exhibiting a noticeable concentration of light towards its center. The core region displays a yellowish-white hue, indicative of an older stellar population. Surrounding the core, a slightly bluer halo suggests the presence of younger stars or ongoing star formation, albeit at a relatively low rate. The galaxy appears largely undisturbed, showing no strong signs of tidal interactions or mergers. There are no prominent spiral arm structures visible, further reinforcing the elliptical classification. The overall shape is moderately elongated, but not significantly cigar-shaped. The smoothness of the light distribution implies a well-mixed stellar population within the galaxy.
