The galaxy presents as a singular, relatively compact object with a generally elliptical morphology. The light profile appears smooth, with a concentrated central region, likely indicating a substantial bulge. A slight color gradient is observed, transitioning from a warmer, yellowish hue in the core to somewhat cooler, subtly bluer tones in the outer regions. There is little evidence of distinct spiral arm structures or significant dust lane features from this limited data. The overall appearance indicates a system that is either spheroidal or an early-type spiral with a dominant bulge.
