The galaxy presents an overall elliptical morphology, though not perfectly round. There's a relatively smooth distribution of light, with a centrally concentrated, bright core that gradually fades into a diffuse halo. The color profile suggests a dominant population of older stars, with a redder hue concentrated in the central bulge and a slightly bluer tinge in the outer regions. No distinct spiral arm structures or dust lanes are discernible. There may be some minor gravitational disturbance or interaction occurring, however it may be the result of image quality. Overall, the galaxy appears to be a relatively massive system undergoing moderate star formation.
