This galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or a potentially active galactic nucleus. Progressing outwards, the galaxy's luminosity gradually decreases. There is a subtle color gradient observed, transitioning from a yellowish-white core to a slightly redder halo, possibly indicative of older stellar populations in the outer regions. Some faint, irregular features, that could be minor disturbances or faint tidal tails are visible, implying that the galaxy may have undergone or is currently undergoing a minor interaction with another galaxy. Overall, the galaxy appears to be relatively isolated with a concentrated bulge.
