This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, indicative of a significant stellar density and possibly a supermassive black hole. Moving outward from the core, the light gradually fades, suggesting a decrease in stellar population density. The isophotes appear elongated, with a cigar-like shape, though not perfectly elliptical. There may be subtle disturbances in the outer regions but overall the galaxy exhibits minimal signs of mergers or major interactions. There appears to be ongoing star formation, as evidenced by a slightly bluer hue in some areas.
