The galaxy presents as a smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests an older stellar population, exhibiting a yellowish-white hue in the central region, likely indicative of evolved stars. The isophotes appear relatively regular, with no discernible spiral arm structure or significant dust lanes. There is a slight elongation in shape. The overall appearance suggests a quiescent system with little active star formation. The lack of blue light further reinforces the assessment of a galaxy dominated by an older stellar population. The object does not display any obvious signs of interaction or recent merger activity, although subtle tidal features could be present but not discernible at this resolution.
