The galaxy exhibits a primarily smooth morphology with a subtle disk-like structure. The central region appears spheroidal and displays a concentrated, bright yellowish-orange hue, potentially indicating an older stellar population. Surrounding this central bulge is a fainter, bluish disk component, suggestive of ongoing star formation. The disk structure shows signs of minor disturbances or irregularities, possibly indicating past interactions or mergers. The galaxy's overall shape appears moderately elliptical, being neither perfectly spherical nor highly elongated.
