The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears to be yellowish-white, suggesting an older stellar population. The galaxy's overall color profile indicates a relatively low rate of current star formation. There are subtle hints of a faint disk extending outwards, though it lacks prominent spiral arm features. The galaxy displays a slight asymmetry, and potential signs of a minor tidal disturbance can be inferred based on the overall morphology. The isophotes show a very slight cigar shape with a small percentage of mergers or disturbance.
