The galaxy appears as a largely featureless elliptical, exhibiting a high degree of central concentration. It has an overall smooth morphology, with no distinct spiral arms or bar structure visible. The color profile suggests a predominantly older stellar population, with a yellowish-white hue that indicates a lack of recent star formation. The galaxy is relatively compact in size, spanning an estimated 6.7 kiloparsecs. There is no clear evidence of ongoing mergers or tidal disturbances affecting its structure. The overall impression is that of a relaxed and evolved system.
