The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile towards the center. The core appears yellowish-white, indicating a population of older stars. The light gradually fades away from the center and begins to take on a bluish tint, suggesting the possibility of some recent star formation. There are no discernible spiral arm structures or dust lanes visible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal distortions. The shape is somewhere between round and cigar-shaped. It is a medium sized galaxy and has a low specific star formation rate.
