The galaxy appears as a relatively smooth, centrally concentrated elliptical morphology. The core exhibits a bright, yellowish-white hue indicative of an older stellar population. The overall shape is not perfectly spherical, displaying a slight elongation suggesting a classification somewhere between elliptical and lenticular. There is a subtle color gradient extending outwards from the center towards a more diffuse, reddish halo. Evidence of spiral arm structure or significant dust lanes is absent. The galaxy does not appear to be undergoing any major merger events, though there may be minor disturbances or interactions observable in the outer regions. The faint outer halo indicates that this galaxy's star formation is not active.
