The galaxy exhibits a predominantly smooth morphology with a discernible central bulge that appears roughly spherical. There's a visible but faint disk component. The color gradient suggests an older stellar population, more yellow and red, particularly concentrated in the bulge. The disk appears slightly bluer. Based on its appearance, this galaxy can be classified as an early-type spiral, with its classification leaning towards lenticular, and shows no strong evidence of ongoing major mergers or significant disturbances. The light is centrally concentrated.
