The galaxy presents as a somewhat elongated, smooth structure with a bright central bulge. The galaxy exhibits a yellow-red hue, suggesting a population of older stars with relatively little ongoing star formation. The overall morphology appears relatively undisturbed, lacking any major signs of tidal tails or ongoing merger activity. The object possesses an approximate effective radius of 6.6 kpc, suggesting it is a galaxy of substantial size. There is a hint of a disk-like structure, with the elongation indicating a possible flattened shape, though this could be a prolate spheroid.
