The galaxy presents a predominantly smooth morphology, suggesting it is likely an early-type system. The overall shape appears somewhat elliptical, falling somewhere between round and elongated. There's no obvious spiral structure or distinct disk component visible; it appears to be a single, largely homogenous light source. The central region is bright and concentrated, displaying a yellowish hue which potentially signifies an older stellar population. Moving outward from the center, the color shifts to a slightly redder tone, potentially indicating the presence of some dust or a slightly younger population of stars in the outskirts. There is no evident tidal debris, strong distortion, or nearby companions, indicating that the system is likely not undergoing any major mergers or strong gravitational interactions at this time, but there is a slight disturbance. There is little apparent star formation activity.
