The galaxy presents as a primarily elliptical or spheroidal structure, characterized by a smooth and centrally concentrated light distribution. A slight elongation is perceptible, though the overall shape appears to be generally rounded. The core region of the galaxy exhibits a yellowish hue, potentially indicative of an older stellar population.

A fainter, smaller region with bluer light is visible on one side of the galaxy. This could indicate a region of recent star formation, a tidal feature resulting from an interaction, or a smaller satellite galaxy. There is no strong evidence of well-defined spiral arms or a prominent disk. The overall color suggests a moderate redshift. There may be a faint disturbance in the galaxy shape, indicating a possible interaction with another galaxy.
