The galaxy presents as a somewhat smooth, disk-like structure, but is viewed at an angle. There is evidence of internal structure, potentially spiral arms or dust lanes, although they are not sharply defined. The central bulge appears relatively prominent and exhibits a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy show bluer tones, possibly indicating regions of more recent star formation, though the overall star formation rate is estimated to be low. The galaxy's shape is more lenticular than perfectly circular, trending towards being cigar-shaped. There might be a very minor interaction with a smaller object or some tidal disturbance, but the overall structure is largely undisturbed, indicating a relatively quiescent state.
