The galaxy presents a generally smooth and rounded morphology. Its light is concentrated towards the center, suggesting a prominent bulge. The color appears somewhat redder than average for galaxies at this distance, hinting at a population of older stars and a relatively low rate of ongoing star formation. There is no obvious spiral structure or bar feature visible. The galaxy appears relatively isolated, with no clear signs of major interactions or mergers, although a very slight asymmetry could possibly be seen on its edges. Overall, the galaxy seems to be an elliptical, at approximately 4.7 kpc in radius, with an estimated stellar mass above 10^10 solar masses.
