The galaxy presents a slightly elongated, elliptical morphology. A bright, concentrated core is visible, suggesting a significant concentration of stars or an active galactic nucleus. The galaxy appears to be relatively smooth in structure, with no prominent spiral arms or obvious dust lanes detected. A subtle color gradient is present, with the central region displaying a slightly bluer hue, possibly indicating a younger stellar population or ongoing star formation activity compared to the outer regions. The overall color is leaning towards blue, indicating a galaxy consisting of new stars. The outer regions of the galaxy fade gradually into the background, indicating a decreasing stellar density with increasing distance from the galactic center. There are no other galaxies or objects around it that seem to be merging with the galaxy, but some small tidal features may be present.