The galaxy appears to be a relatively smooth, elliptical-type system. Its morphology is dominated by a central bulge that exhibits a yellowish-orange hue, indicative of an older stellar population. Surrounding the bulge is a less concentrated halo with a bluer tint, hinting at the presence of some younger stars or perhaps ongoing star formation. The galaxy has a somewhat elongated, cigar-like shape, as opposed to being perfectly spherical. There is no clear evidence of strong tidal features or major disturbances; however, subtle irregularities in the outer regions might suggest minor gravitational interactions or past merger events.
