The galaxy presents as a centrally concentrated, elliptical or lenticular type. It exhibits a smooth, diffuse morphology with a bright, yellowish core that gradually fades towards its periphery. There is no apparent spiral arm structure or dust lane obscuration visible in this image. The shape appears to be fairly regular, exhibiting a close to circular or slightly elongated form. There is no indication of any major tidal disturbance or ongoing merger events. Color gradients are subtle, with a tendency toward bluer hues at the outer regions indicating a slightly younger stellar population compared to the core. Overall, the galaxy's luminosity is considerable, indicating a high stellar mass.
