The galaxy appears to be a relatively smooth, centralized structure. There is a dominant central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. Some faint disk-like features may be present, but the overall morphology is dominated by the central bulge. There are hints of a slight disturbance or faint, diffuse extensions, perhaps due to minor gravitational interactions or past merger events. The galaxy's color suggests a moderate amount of star formation, though it could also be heavily influenced by older stars within the bulge.
