The galaxy presents as an elliptical or lenticular type, displaying a generally smooth morphology with a high degree of central concentration. The light profile transitions smoothly from the core outwards, indicating a lack of prominent spiral arms or distinct features typically associated with disk galaxies. The color gradient suggests a relatively homogenous stellar population. A somewhat centrally located area of brighter, yellowish-white light, likely the galactic bulge, fades into a bluish halo surrounding the core. There is no strong indication of a recent major merger event, tidal tails or strong morphological disturbances. The object is highly symmetrical, leaning more towards round than cigar shaped. Based on the color, there may be weak ongoing star formation.