The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a bright, concentrated luminosity, indicative of a substantial central mass concentration. The overall color appears to be yellowish-reddish, suggesting an older stellar population with fewer young, blue stars. There is a subtle decrease in brightness as you move from the center to the outer edges, though no distinct spiral arms or features are visible. The galaxy appears somewhat elongated, but not extremely so, and appears to be relatively isolated, with no obvious signs of major tidal disruption or interaction with other galaxies in the immediate vicinity. There may be signs of a minor disturbance, but it is hard to tell from this image.
