The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge, surrounded by a more diffuse halo. There is no apparent spiral arm structure, but a faint, disky component may be present. The galaxy appears moderately luminous with redder hues concentrated in the central bulge, suggesting an older stellar population.  The galaxy appears largely undisturbed, with no obvious signs of a major merger event, though there may be some minor asymmetry visible in the outer regions. The overall morphology suggests a galaxy in a late stage of evolution.
