The galaxy presents a predominantly smooth morphology. The overall shape appears nearly circular, exhibiting a high degree of roundness. There is no clear evidence of spiral arms or a defined disk structure. The light is mostly concentrated centrally, with a gradual decrease in intensity towards the outer regions. The primary color of the galaxy's core appears to be greenish-white, possibly indicating a high concentration of ionized gas or younger stellar populations. A secondary, smaller object is observed nearby, exhibiting a more reddish hue. This may indicate an older stellar population, or that it is further away. There is a small chance that it is interacting with the primary galaxy, but no clear signs of tidal tails or distorted morphology are immediately apparent to suggest a major interaction or merger event. The galaxy appears relatively undisturbed.
