The galaxy presents as a single, relatively smooth and compact object with a concentrated central region. The color appears yellowish-orange, which suggests an older stellar population with relatively low levels of ongoing star formation. Morphologically, it appears to be transitioning from a smooth elliptical galaxy to a merging system. There is a slight elongation or distortion in its overall shape, possibly indicating the presence of a minor interaction. The system's structure reveals a primary central concentration surrounded by fainter, extended material. The galaxy does not exhibit clear spiral arm structures or prominent dust lanes.
