The galaxy presents a relatively smooth, elliptical morphology, with a bright, concentrated central bulge. The luminosity profile appears to decrease smoothly outward from the core, suggesting a lack of distinct spiral arm structures. The overall shape is somewhat elongated, deviating slightly from a perfect circle, indicating an intermediate form between round and cigar-shaped. There are subtle asymmetries in the outer regions of the galaxy, possibly indicative of minor gravitational disturbances or interactions. While no major merger events are immediately apparent, the slight irregularities might suggest past or ongoing minor interactions. The color indices hint at a redder overall population, consistent with an older stellar population and suppressed star formation.
