The galaxy presents as a generally smooth, centrally concentrated object. The light distribution suggests a dominant spheroidal component with a relatively high degree of circularity. There is a lack of apparent spiral arms or a distinct disk-like structure, as evidenced by its homogenous, smooth appearance. The galaxy exhibits a noticeable color gradient, with a yellowish hue dominating the central region and an apparent reddening towards the outer edges. This color gradient could indicate a radial variation in stellar populations or dust content, with older, redder stars potentially residing in the outer regions. Faint tidal features or minor disturbances are possibly present but are not clearly defined. The galaxy does not appear to be strongly interacting with other galaxies in its immediate vicinity, based on the absence of obvious tidal tails or bridges. Overall, this galaxy appears to be a relatively quiescent system, potentially an elliptical galaxy at intermediate redshift.
