The galaxy presents as a centrally concentrated, elliptical-like object. It exhibits a smooth, largely featureless morphology with no apparent spiral arm structure or dust lanes visible at this resolution. The color profile shows a dominant yellow hue, suggestive of an older stellar population. The galaxy appears relatively isolated, with no immediately apparent signs of major tidal disturbances or ongoing mergers, although subtle distortions or minor interactions cannot be entirely ruled out. The apparent roundness suggests a possible E0-E3 classification on the Hubble scale.
