The galaxy presents as a luminous, elliptical-type object. It exhibits a smooth, centrally concentrated luminosity profile, with a gradual decrease in brightness from the core outward. There is a slight elongation visible, indicating a shape that is neither perfectly spherical nor highly flattened. The overall color appears to be on the redder end of the spectrum, suggesting an older stellar population and reduced ongoing star formation. No prominent spiral arm structures or significant dust lanes are discernible, implying a relatively quiescent state with minimal recent merger activity or starburst events. The galaxy displays a hint of disturbed morphology, possibly a tidal feature extending from the galaxy. The size is relatively compact.
