The galaxy presents as an elliptical type, with a smooth, concentrated light distribution that gradually fades toward its periphery. The central region exhibits a brighter, yellowish hue, suggesting an older stellar population and less ongoing star formation in that area. The outer regions display a more subdued, bluish tint, which may indicate the presence of younger stars, although this is less pronounced. There is a slight asymmetry noted at the very edge, with what looks like a small disturbance on the bottom left. There are no obvious spiral arms or prominent dust lanes are detected. The overall morphology suggests a relatively evolved system with low to moderate star formation activity.
