The galaxy appears to be a relatively smooth, elliptical-type system. Its overall form presents a rounded morphology with a slight extension along one axis, though not strongly cigar-shaped. The galaxy displays a prominent central bulge that is more luminous and yellow in color, suggesting an older stellar population in the core. Fainter, bluer light extends outwards from this central region, hinting at some level of ongoing star formation activity. There is a faint possibility of a minor disturbance or irregularity in its outer structure, but it appears largely undisturbed. There's no definitive evidence of a major merger.
