The galaxy appears to be an elliptical galaxy, showing a relatively smooth and concentrated light distribution. It exhibits a generally round morphology, with a slight elongation. The central region is characterized by a bright, yellowish hue, likely indicative of an older stellar population. The outer regions fade into a more diffuse halo with a hint of bluer light, suggesting a small amount of recent or ongoing star formation. No obvious spiral arms, bar structures, or major disturbances are discernible. There is no clear evidence of a major ongoing merger. Overall, it presents a well-defined, evolved system.
