The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable color gradient, transitioning from a bright, yellowish core to a redder, less defined halo. No spiral arm structures or dust lanes are immediately apparent. The galaxy appears to be relatively isolated, showing no signs of major tidal disturbances or ongoing mergers. The overall morphology suggests a well-evolved system, potentially dominated by an older stellar population, although some ongoing star formation is still likely present within the galaxy.
