The galaxy presents as a relatively smooth, elliptical object with a slight elongation along its major axis. The central bulge is prominent, exhibiting a concentrated brightness and a yellow-red hue, suggestive of an older stellar population. A fainter, more diffuse halo surrounds the central bulge. There is some evidence of a disk, indicated by a subtle flattening and a slight color gradient moving outwards from the center. The outer regions display a bluish-green tint, potentially indicating the presence of younger, hotter stars and ongoing star formation activity, though at a low rate. No strong spiral arm structures are visible, nor are there obvious signs of a major merger event, although there may be subtle signs of a minor disturbance in the galaxy's overall structure. The morphology appears to be somewhere between a perfect circle and a cigar shape, though with a strong lean toward roundness. The galaxy exhibits a moderate mass, and an absolute magnitude that suggests a luminous object at its distance.
