The galaxy presents as a relatively smooth, elliptical-shaped structure with a noticeable bulge. Its color profile is primarily yellow/gold in the central region, suggesting a population of older stars, while the outer edges exhibit a slight blue tint, possibly indicating ongoing or recent star formation. The overall light distribution is concentrated towards the center, with a gradual fall-off in intensity towards the edges. The galaxy appears elongated, with an axial ratio suggesting it is not viewed face-on. There is no evidence of spiral arms or a disk structure. There is little to no morphological disturbance apparent, indicating no ongoing major merger activity.
