The galaxy presents a generally smooth morphology with a central, concentrated bulge. This bulge exhibits a yellowish-white color, suggestive of an older stellar population. The overall shape is elliptical, but not perfectly so, as the isophotes are not perfectly circular. A faint disk-like structure is barely perceptible around the bulge, oriented roughly horizontally in the image. This structure is bluer in color than the bulge, hinting at ongoing star formation. One region on the right of the galaxy has an orange tinge, possibly indication of an area of dust obscuration or a different stellar population. There is no clear sign of strong tidal features or major merger activity, though minor disturbances cannot be ruled out. The galaxy appears relatively isolated.
