This galaxy presents a relatively smooth, elliptical morphology, exhibiting a centrally concentrated light profile. The core region displays a bright, yellowish-orange hue, possibly indicative of an older stellar population dominating the nuclear region. There is a slight extension or disturbance that may hint at either a tidal feature or early stages of a minor merger with another galaxy. The light distribution is consistent with a relatively low level of ongoing star formation overall. The galaxy appears to be roughly spheroidal in shape with hints of elongation and tidal disruption, although the resolution limits a more precise determination of the underlying structure. 
