The galaxy presents a largely smooth, elliptical morphology. The light distribution appears concentrated toward the center, exhibiting a bright, roughly spherical core. Moving outward from the core, the light gradually diffuses into a fainter, elongated halo. The major axis of the galaxy is noticeably longer than the minor axis.

The color profile indicates an older stellar population. The core exhibits a yellowish-orange hue, suggesting a dominance of evolved stars. There is no apparent presence of dust lanes or prominent spiral arm structures. The outer regions of the galaxy show a subtle shift towards redder colors, possibly indicative of a decreasing age of the stellar populations toward the galactic fringes.

The overall appearance suggests a relatively undisturbed system with minimal signs of recent mergers or tidal interactions. Any internal structure is obscured by distance and a generally smooth distribution of stars.
