This galaxy presents as a largely featureless, elliptical structure. Its overall shape is predominantly round, exhibiting high central concentration. The light profile appears smooth, with minimal evidence of spiral arms, bars, or distinct morphological features. A faint blue hue permeates the central region, possibly indicating the presence of a moderate population of relatively young, hot stars. The outer regions show a gradual decrease in intensity and reddening, suggestive of an older stellar population dominating the halo. There appears to be no significant tidal disturbance or clear signs of a major ongoing merger event.
