The galaxy presents as a fairly smooth, elliptical structure. It exhibits a concentrated central bulge that appears yellowish-white, suggesting an older stellar population. The outer regions of the galaxy are less defined, fading into the background with a subtle blueish tinge. The morphology is dominated by the smooth central region with minimal visible spiral arm structure or distinct features, indicating an absence of substantial recent star formation. Overall, the galaxy appears to be relatively isolated and undisturbed with little evidence of major interaction with other galaxies or merging events.
