The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, suggesting an older stellar population. The galaxy's overall shape is somewhat elongated, appearing neither perfectly spherical nor disk-like. A faint, diffuse halo surrounds the central region, gradually fading into the background. There is no apparent evidence of spiral arms or significant dust lanes. Subtle irregularities may suggest a minor gravitational disturbance, but no clear signs of a major merger are present. Star formation appears to be subdued.
