The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge is evident, exhibiting a yellowish hue. A diffuse halo surrounds the core, transitioning from yellow at the center to redder tones towards the outer regions. There is a subtle hint of disk-like features, but no prominent spiral arm structure is discernible. The overall appearance suggests a system undergoing relatively low levels of star formation, with the bulk of the stellar population likely comprised of older, redder stars. There is no evidence of major mergers or significant tidal disturbances. The galaxy's shape appears close to round.
