The galaxy presents as a somewhat elongated, diffuse structure, suggesting an elliptical morphology, though the possibility of a highly inclined disk galaxy cannot be entirely ruled out. Its core region exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward from the core, the galaxy fades into a more bluish tint. The overall smooth appearance suggests that any recent major mergers are unlikely. There is some indication of minor asymmetry or a slight disturbance in its morphology. The galaxy does not have distinct spiral arms. The galaxy appears relatively isolated, although higher resolution imaging would be required to confirm the absence of faint tidal features or nearby dwarf galaxies. 
