The galaxy presents as a generally smooth object, with a high degree of circular symmetry. The light profile exhibits a concentrated central bulge that fades gradually into the outer regions of the galaxy. A slight elongation is perceptible, hinting at a possible elliptical morphology. The overall color of the galaxy appears to be yellowish-orange, suggestive of a stellar population dominated by older, redder stars. There is no discernible spiral arm structure or dust lanes within this galaxy from this viewing angle. The apparent size of the galaxy suggests it is a somewhat massive system, consistent with the high degree of smoothness and lack of active star formation regions. There seems to be no signs of major ongoing mergers, but a slight irregularity could indicate past minor interactions.