The galaxy presents a generally smooth morphology, with a high degree of central concentration. The overall shape is close to circular when viewed from our perspective, exhibiting slight elongation. The core region is significantly brighter than the surrounding areas. There appears to be a minor disturbance or possible merger event underway, as evidenced by a faint tidal tail-like feature extending from the main body of the galaxy. Based on the color profile, the galaxy appears to have a mixture of stellar populations. There are possibly some younger, bluer stars present, though the dominant population appears to be older, redder stars, especially within the central bulge. The galaxy is relatively large with a significant estimated stellar mass. While it exhibits a low rate of active star formation, indicating it is likely in a quiescent state, the outer regions and the tidal feature have a hint of blue, potentially indicating more recent star formation in those areas.
