This galaxy exhibits a generally smooth morphology, with a concentrated central region that appears yellowish-white, possibly indicating an older stellar population or dust obscuration. There is a subtle extension of bluer, less concentrated light surrounding the core, suggesting the presence of a disk-like structure where active star formation may be occurring. Faint features resembling tidal disturbances are present, indicating past or ongoing interactions with another galaxy. The galaxy's overall shape is closer to an intermediate elliptical, not perfectly round but also not highly elongated. There are hints of disturbed or disrupted galactic structure, implying the galaxy is in a transitional phase, perhaps between a spiral and elliptical type, or undergoing a minor merger.
