The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a lack of prominent spiral arms or significant dust lanes. It is mostly a bright yellow, indicating an older stellar population. The object is elongated, implying that it is most likely a lenticular galaxy. No tidal tails or close companion galaxies are discernible, suggesting the galaxy is relatively isolated or is not currently undergoing a major merger event. There is some suggestion of slight disturbances in the outer parts of the galaxy, but no clear sign of a merger.