The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and diffuse light distribution. It presents an oval shape, with a noticeable flattening. The central region is significantly brighter and yellower than the outer parts, suggesting a concentration of older stars. The color gradient indicates a likely variation in stellar populations across the galaxy, from a more aged core to slightly bluer edges. There is no visible evidence of spiral arms or distinct dust lanes. It looks like the galaxy is not undergoing any major merger events.
