The galaxy presents as a somewhat elliptical object with a concentrated central bulge. The color profile suggests an older stellar population, dominated by yellow and red wavelengths.  There is a slight disk-like structure apparent, though it is not sharply defined. The light distribution is relatively smooth, with no prominent spiral arms or significant dust lanes visible. The outer regions of the galaxy gradually fade into the background, indicating a lack of active star formation in the periphery. Overall, the morphology is consistent with an early-type spiral or an elliptical galaxy.
