The galaxy appears to be a relatively smooth, elliptical system. It exhibits a slightly elongated morphology, exhibiting an axial ratio that suggests it is an oblate spheroid, but tending towards a more circular shape than a cigar shape. A prominent central bulge is observed, characterized by a yellowish hue, likely indicative of an older stellar population dominating this region. Fainter, bluer emission extends from the central region, suggesting the presence of a younger stellar population with ongoing or recent star formation activity. The overall structure lacks any clear spiral arms or significant morphological disturbances, suggesting it is a fairly relaxed system. The galaxy doesn't show any signs of a major merger event, it may show some minor disturbances.
