The galaxy presents as a relatively smooth, elliptical structure. Its overall form is somewhat elongated, tending towards a cigar shape rather than perfectly circular. A distinct central bulge is visible, exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions appear less concentrated, with a bluer tint that potentially indicates the presence of younger stars and ongoing star formation, although at a low rate. There is no obvious indication of spiral arms or a prominent disk-like structure. There is also no significant presence of tidal tails or merging evidence to suggest a major merger. The galaxy exhibits a relatively undisturbed morphology.
