The galaxy presents a generally smooth, rounded morphology. There is a distinct, centrally concentrated bulge region that exhibits a bright, yellowish-white hue. This central region appears relatively featureless at this resolution, suggesting an older stellar population. A faint, diffuse halo or envelope surrounds the central bulge, exhibiting a slightly bluer coloration. The galaxy displays no prominent spiral arm structures or distinct dust lanes that can be clearly identified in this image. There are slight disturbances in the outer halo, hinting that there might be a minor merging event occurring.
