The galaxy presents a generally smooth and elliptical morphology. It appears to be a relatively bright object, with a concentrated central bulge that transitions into a fainter, more diffuse halo. The galaxy exhibits a slight elongation, deviating from a perfect spherical shape. There is a subtle color gradient, with the core exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. The outer regions appear somewhat bluer, which may be due to the presence of younger stars. There is no clear evidence of spiral arms, bars, or significant dust lanes. The galaxy does not appear to be undergoing any major mergers or interactions.
