The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated morphology without discernible spiral arms or distinct features. It appears moderately elongated, approximately cigar-shaped, with the major axis exceeding the minor axis. The central region shows a high concentration of light, suggesting a substantial galactic nucleus or bulge. The colouration is generally yellowish-white, indicative of an older stellar population. Some minor asymmetry is observed suggesting potential past interactions or minor disturbances, though there are no clearly defined tidal tails or merging features. The overall structure appears mostly undisturbed and relatively evolved.
