This galaxy appears to be a relatively face-on spiral with a prominent bulge. The bulge region exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population. The surrounding disk shows evidence of spiral arms. There is a slight color gradient from the center outwards, with the core being more yellow-white and the outer regions tending towards bluer tones. No significant dust lanes are visible, and the spiral arms are somewhat loosely wound. Overall, the galaxy appears undisturbed, without any obvious signs of major mergers or tidal interactions.
