The galaxy presents an elliptical morphology, exhibiting a dominant, centrally concentrated spheroid component. The overall structure is characterized by a smooth light distribution, with minimal visible substructure. The central region displays a bright, relatively homogenous luminosity profile suggestive of an older stellar population. The object's light profile appears moderately round. There are some hints of possible tidal features or minor disturbances in the outer halo regions, although this interpretation is tentative given image resolution. There is also the possibility of merger activity happening. The galaxy exhibits colors that are consistent with a galaxy at intermediate redshift, showing colors in green, red, and some blue.
