The galaxy presents as a centrally concentrated, diffuse object. Its morphology appears largely smooth with little to no discernible spiral arm structure or pronounced features. The galaxy exhibits a slightly elliptical shape, and the color is indicative of an older stellar population, with a blue hue most visible. There is no evidence of a bright, active galactic nucleus, tidal tails, or strong dust lanes, suggesting a relatively quiescent state. The overall visual impression is that of an early-type galaxy, possibly an elliptical or lenticular galaxy viewed at a considerable distance. There may be very minor disturbances, but its merger fraction is quite small. 
