The galaxy presents a generally smooth, elliptical morphology. The light is concentrated towards the center, indicating a prominent bulge. A slight extension can be seen along one axis, possibly indicating a mild elongation or the beginning of a disk-like structure. The color appears yellowish-orange, suggesting an older stellar population with relatively little ongoing star formation. There is no obvious evidence of spiral arms, dust lanes, or significant irregularities in the galaxy's structure, implying a settled, evolved system. There is no visible presence of any tidal disturbances or ongoing merger activity.
