The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution appears fairly uniform, indicating an older stellar population dominating the light output. There is a faint, diffuse halo surrounding the central region, gradually fading into the background. Subtle color gradients are present, shifting from a yellow-orange core toward a slightly bluer periphery. There is no clear evidence of spiral arms, dust lanes, or ongoing major star formation. Based on the lack of significant morphological distortions, the galaxy is likely undisturbed, with no signs of recent major mergers, but may have minor disturbance from possible minor mergers. The galaxy is roughly symmetrical, with an approximately round shape, displaying a slight elongation.
