The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It exhibits a concentrated central bulge with a moderate radial gradient in surface brightness. The galaxy displays a yellowish hue, potentially indicating an older stellar population with a lower rate of ongoing star formation. No distinct spiral arm structures or dust lanes are apparent in the image, indicating a lack of significant star formation. It exhibits a slight asymmetry but seems to be relatively undisturbed by any major merging events. The roundness of the galaxy appears to be somewhere in between completely round and slightly elongated. Overall, the galaxy presents a general morphology consistent with an evolved system dominated by older stars.
