The galaxy presents a relatively smooth, elliptical morphology. It is elongated, appearing cigar-shaped. The light distribution is concentrated towards the center, indicating a prominent bulge. There is a color gradient, with the central region appearing yellowish-white, suggesting an older stellar population. The outer regions exhibit a bluer tint, hinting at the presence of younger stars, but the overall star formation activity appears low. There is no obvious evidence of spiral arms or significant dust lanes. No signs of major mergers are evident. Faint, minor disturbances may be present, but it's difficult to ascertain without higher resolution imaging.
