The galaxy presents as a roughly elliptical structure with a concentrated central bulge. The core exhibits a bright, relatively uniform luminosity, suggesting a high density of stars. Surrounding the core is a more diffuse halo that appears mostly smooth, though faint, irregular features are present within it. There is some indication of a slight disk structure but not highly pronounced. Color gradients indicate younger stars and some ongoing star formation within the outer regions of the halo, though it appears overall subdued. There is no immediately apparent evidence of active galactic nuclei activity or strong tidal disturbances from interactions with other galaxies.
