The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. A subtle color gradient is observed, transitioning from a yellowish-white core to a bluer, less intense outer halo. There's little indication of distinct spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved system, potentially undergoing less active star formation compared to disk galaxies. The roundness of the observed shape may indicate a nearly face-on orientation, with no obvious signs of major mergers or tidal disturbances. The galaxy's smooth appearance and color profile are consistent with an older stellar population, possibly dominated by redder giant stars.