The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that displays a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy appear more diffuse, fading into the background sky. These regions show a hint of bluer light, possibly indicating the presence of younger, hotter stars, although their number appears relatively small. The galaxy does not exhibit any distinct spiral arm structures or a prominent disk. There is some indication of minor disturbances in its shape, perhaps due to a past interaction or merger. The overall light distribution suggests that this galaxy is moderately massive.
