The galaxy presents as an elliptical-type system. It exhibits a smooth, centrally concentrated light profile, transitioning outwards into a diffuse halo. The major axis appears significantly longer than the minor axis, giving it a somewhat elongated, cigar-shaped appearance. There's a subtle color gradient visible, trending from a yellowish-white core to a bluer outer region, possibly indicating differing stellar populations or dust distribution. No distinct spiral arm structures or major disturbances indicative of an ongoing merger are readily apparent. The overall morphology suggests a relatively evolved, quiescent system. There might be very minor signs of tidal disruptions, but further observations are necessary to determine if any mergers are occuring.
