The galaxy presents a largely smooth, elliptical morphology with a prominent central bulge. The core exhibits a bright, concentrated luminosity that gradually diminishes outward. The overall shape appears somewhat elongated, deviating slightly from a perfectly circular form. There are faint indications of asymmetry, but no obvious spiral arm structures are visible. The galaxy's color profile shifts from yellow-white in the core to a redder hue towards the outer edges, which might suggest differing stellar populations or dust distribution. There is no evidence of any major merger events or tidal disturbances impacting the galaxy's form, although there may be some evidence of minor disturbance. There appears to be very little in the way of star formation occurring within the galaxy.
