The galaxy presents as a moderately bright, well-defined elliptical or lenticular structure. It exhibits a smooth, centrally concentrated light distribution, suggestive of an evolved stellar population. There is some evidence of a slight elongation in its morphology, deviating from a perfectly circular shape. It appears relatively undisturbed, showing no strong signs of tidal interactions or ongoing merger activity. The color profile indicates the presence of older stars, giving off yellowish light. There might be slight hints of blue light suggesting some areas of star formation activity, however faint.
