The galaxy presents as an elliptical-like structure, with an approximate visual diameter of 3.6 kpc. The core appears to be a concentrated luminosity, possibly indicating a substantial central mass concentration. The morphology is smooth, with a relatively high degree of roundness but leaning toward an elongated shape. There may be some minor disturbance in its outer structure, though the image isn't conclusive. The galaxy has a color gradient. The center is yellowish-white, fading to a slightly bluer hue towards the edges. The galaxy does not seem to show strong evidence of being involved in a major merger. Star formation rate is low, likely consisting primarily of older stars. The overall structure doesn't show a disk.
