The galaxy exhibits a primarily smooth morphology with a slightly elliptical shape. The central region displays a concentrated, bright luminosity, suggesting a prominent galactic nucleus. The color profile shifts from a yellowish-white core to a bluer halo, indicating a potential variance in stellar populations, with the core possibly dominated by older, redder stars and the halo containing younger, bluer stars. There appears to be little evidence of spiral arm structures or significant dust lanes. There might be a slight disturbance in the evenness of the light from the galaxy, although this is probably due to the resolution of the image.
