The galaxy presents as a lenticular or early-type spiral, exhibiting a predominantly smooth and featureless structure. Its overall shape is elliptical, with an aspect ratio suggesting a moderate degree of flattening, but is closer to round than cigar shaped. There's a distinct central bulge, characterized by a high surface brightness. The bulge appears nearly spherical, while the disk component is less obvious. Subtle color gradients can be observed, with a slightly bluer tint in the outer regions compared to the yellower-redder central bulge, potentially indicating some ongoing or recent star formation. No prominent spiral arms, dust lanes, or signs of active galactic nuclei are readily apparent. There is no evidence of any significant merger events or tidal disturbances in the galaxy's immediate vicinity.
