The galaxy presents a largely smooth, elliptical morphology. There is a high degree of circular symmetry observed. No prominent spiral arms or bar structures are apparent within the limits of resolution. The central bulge appears dominant and smoothly transitions to a fainter, diffuse halo. The light profile appears concentrated. There is some minor indication of possible tidal features or faint disturbances in the outer regions, possibly indicating interaction or accretion events, though this is uncertain given the image quality. The galaxy exhibits a reddish color, suggesting an older stellar population, with a relatively small amount of on-going star formation. The galaxy's overall structure is largely unperturbed, showing no indication of an ongoing major merger.
