This galaxy exhibits a generally smooth morphology, with some faint features suggestive of a disk-like structure or possible disturbances. The central region is brighter and more condensed than the outer regions. The color appears to be bluish-white, which could indicate a significant population of younger, hotter stars. The overall shape is somewhat irregular, showing some deviation from a perfect elliptical or spiral form, perhaps due to interactions with another galaxy. There may be indications of minor disturbances within the galactic structure.
