The galaxy presents as a concentrated, elliptical form with a smooth overall appearance. A central bulge of moderate luminosity dominates the structure, exhibiting a yellowish-white hue. Moving outward from the core, the galaxy appears more diffuse and less defined. There are faint hints of disk-like structure, but with no distinct spiral arm features visible. The shape of the disk appears neither perfectly circular nor highly elongated. The light distribution suggests a relatively evolved system, with low levels of ongoing star formation. There is no evidence of strong tidal interactions or major mergers; any disturbances appear minor.
