The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. The central region exhibits a concentrated luminosity, with a gradual decrease in brightness towards the outer edges. The overall color is primarily reddish-yellow, possibly indicating an older stellar population with lower levels of ongoing star formation. There is minimal evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or merging events, though a slight distortion may be present. The general form indicates a possible spheroidal system with little disk component.
