The galaxy appears as a largely smooth, centrally concentrated object. It exhibits an elliptical morphology, with an apparent lack of spiral arm structure. The central region presents a yellowish hue, possibly indicative of an older stellar population. Fainter, bluer light is observed extending outwards from the core. The overall smoothness and color distribution suggests that star formation may be occurring, though at a moderate rate. There is a slight suggestion of possible minor tidal disturbances or interactions, however the primary structure is smooth.
