The galaxy presents as a moderately bright object with a generally smooth appearance. It appears to be lenticular, with a central bulge and a faint disk. The bulge exhibits a yellowish hue, transitioning into a bluish disk, indicating differing stellar populations. There is no clear evidence of spiral arm structure. The galaxy exhibits a slight elongation; it is of intermediate roundness. There is no obvious major merger or significant tidal distortion, although it shows signs of a minor disturbance. The overall color suggests relatively recent or ongoing star formation, yet a notable fraction of its light seems to be derived from an older stellar population, as indicated by the yellow bulge. The galaxy is relatively compact and the concentration of light is high.
