This galaxy presents as a roughly elliptical, disk-shaped structure. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. A flattened disk extends outward from the core. The disk appears relatively smooth, showing little evidence of prominent spiral arm structure or significant dust lanes. Color variations suggest potential differences in stellar populations or dust distribution. The central region appears bluer, possibly indicating a younger stellar population or less dust obscuration compared to the outer regions, which exhibit a slightly redder hue. There are subtle irregularities in the outer regions that could suggest minor gravitational interaction or disturbance, but otherwise it is relatively uniform. Overall, the galaxy appears to be in a relatively relaxed state.
