The galaxy presents a largely smooth morphology, appearing as a somewhat rounded, concentrated structure. The light distribution suggests an elliptical or lenticular morphology, with a centrally concentrated bulge. There is evidence of possible tidal features, but the image resolution makes these observations ambiguous. The galaxy exhibits a redder color, implying an older stellar population and relatively suppressed star formation. There appears to be a possible minor disturbance or merger event in progress, as the structure of the galaxy is slightly distorted.
