The galaxy presents as an elliptical or lenticular type. It exhibits a centrally concentrated bulge that appears smooth and largely featureless, with a yellow hue, potentially indicating an older stellar population. There's a slight elongation to the galaxy's overall shape, moving into a cigar shape. There is also a slight disk-like structure. Hints of fainter, bluer light extending from the central region suggest the presence of some ongoing star formation or a younger stellar component. There are no clear signs of strong spiral arms or major disturbances, and no merger events are visible. The outer edges appear diffused and without any noticeable irregularities or tidal tails.