The galaxy presents as an elliptical morphology, with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The overall light distribution appears smooth and relatively featureless. There is a slight elongation noticeable along one axis, giving it a somewhat oblate appearance. Faint, diffuse light extends outwards from the core, fading into the background. There is no obvious disk structure or spiral arms visible. No indications of major mergers or tidal disturbances are apparent in the immediate vicinity of the galaxy.
