The galaxy appears to be a relatively smooth, centrally concentrated system. It presents a roughly elliptical morphology, appearing more "in between" rather than distinctly round. The galaxy exhibits a gradual fading from a bright core to a diffuse outer region, lacking sharp edges or distinct spiral arm structures within the limitations of this image resolution. There are suggestions of faint, diffuse features, possibly indicating some mild gravitational disturbance but with no signs of major merging activity. The color gradient suggests a population of older stars toward the center, with possibly a small amount of star formation that is not easily discernable.
