The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears reddish, transitioning into a yellowish halo. There is no apparent spiral arm structure or bar feature visible. The galaxy is relatively isolated; no other galaxies appear to be in the process of merging or interacting. The outskirts of the galaxy seem devoid of significant dust lanes or distinct features. The overall color index is redder in the core, suggesting an older stellar population dominating that region, while the outer halo exhibits slightly bluer tints, which may indicate the presence of younger stars. The roundness of the galaxy indicates a more even mass distribution, with no particular distortions suggestive of past merger events.