The galaxy presents a generally smooth, elliptical morphology, although not perfectly round. A concentrated central bulge dominates the structure, exhibiting a distinct reddish-orange hue suggesting an older stellar population. Surrounding the bulge is a less defined disk or halo component, displaying a bluer color profile indicative of more recent star formation. Faint wisps or arm-like features are barely discernible within this outer region. No apparent dust lanes or significant irregularities are noted, but some minor disturbance cannot be ruled out. The overall light distribution is centrally concentrated, decreasing gradually towards the outer edges.
