The galaxy presents a somewhat elliptical morphology, with a noticeable, though not sharply defined, central bulge. It appears relatively smooth in overall texture. The colour profile exhibits a shift towards redder hues in the central region, potentially indicating an older stellar population in the bulge. Fainter bluer regions appear towards the edges. There may be very subtle evidence of a disk structure, but it is difficult to ascertain. No prominent spiral arms or significant dust lanes are visible. There do not appear to be any signs of significant disturbances or ongoing merger activity.
