The galaxy appears as a relatively compact, elliptical system with a smooth, diffuse light profile. The core exhibits a concentrated brightness, suggesting a high stellar density. The overall color is a yellowish-orange hue, indicative of an older stellar population with a lower rate of active star formation. There is a slight asymmetry to the galaxy's shape, leaning more to a flattened spheroid than a perfect circle. A very faint, bluish tinge is observed in the outer regions, hinting at some residual star formation, albeit at a low level. There are no apparent spiral arms or dust lanes visible. The general morphology suggests this is likely an evolved galaxy undergoing minimal recent interaction or major merger events.
