The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge exhibiting a yellow-white hue, indicative of an older stellar population. This core is surrounded by a fainter, more diffuse halo exhibiting a slight blue tint, potentially indicating a small amount of recent star formation, or at least a population of younger, bluer stars. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears largely undisturbed, with no prominent signs of ongoing or recent major mergers or tidal interactions. The overall morphology suggests a galaxy transitioning towards a quiescent state, with the majority of star formation having ceased.
