This galaxy exhibits a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The color gradient is relatively uniform, with a yellowish hue dominating the central region, possibly indicative of an older stellar population. There is no discernible spiral arm structure or obvious dust lanes. Faint hints of tidal disturbances or minor asymmetries are present in its outer halo, particularly toward the right, possibly indicating a past minor merger event. The galaxy appears relatively isolated in this image, with no other galaxies in close proximity. The overall characteristics suggest a relatively massive galaxy with a moderate star formation rate and a significant degree of spheroidal symmetry.
