The galaxy presents as a relatively smooth, lenticular structure. It exhibits a prominent central bulge that is slightly elongated. The color of the bulge is generally a yellowish-orange hue, which may indicate an older stellar population dominated by red giant stars. A very faint disk surrounds the bulge, with hints of a bluer color, which could indicate a younger stellar population or a region of ongoing star formation, but it is relatively insignificant. There are slight asymmetries visible and a subtle distortion, which suggest a possible minor interaction or disturbance. No prominent spiral arm structures or dust lanes are apparent. The overall morphology suggests an intermediate stage in galaxy evolution, where the galaxy has exhausted much of its gas supply and star formation is suppressed.
