The galaxy presents as a largely featureless, smooth elliptical or lenticular galaxy. A luminous core is visible, with intensity decreasing gradually towards the outer regions, indicative of an older stellar population and the absence of significant dust lanes or spiral arm structures. The galaxy exhibits an intermediate level of roundness and a notable lack of any major merger activity or significant disturbances in its morphology. The color profile shows a general redder hue, possibly consistent with galaxies exhibiting low ongoing star formation rates.
