The galaxy presents a generally smooth appearance with a slight elongation, suggestive of a possible elliptical morphology. There is no clear indication of spiral arms or a prominent disk structure. The light distribution appears centrally concentrated, though the limited resolution makes a definitive determination challenging. The galaxy exhibits a color gradient, with a yellowish-white hue dominating the central region, potentially indicating an older stellar population. Fainter reddish hues appear at the bottom, possibly suggesting ongoing star formation in those regions. The overall structure appears relatively undisturbed, showing no signs of major mergers or tidal interactions. A subtle asymmetry is present in the light distribution, warranting further investigation to determine if it results from a minor interaction or internal processes.
