The galaxy presents a somewhat amorphous structure. While a generally smooth appearance dominates, subtle features suggest ongoing or recent gravitational interaction. A slight extension or tidal tail-like structure is visible on one side, indicating a possible disturbance or merger event. The galaxy exhibits a range of colors, suggesting a mix of stellar populations. The central region appears slightly redder, which could be due to an older, redder stellar population or dust obscuration. Bluer regions are also present, possibly indicating areas of active star formation. The overall shape is somewhat irregular, with deviations from a perfect elliptical or spiral morphology.
