The galaxy presents as a centrally concentrated object, exhibiting a smooth overall morphology. The light distribution suggests a spheroidal component dominating its structure. There is a slight elongation of the central region. The galaxy displays a color gradient, appearing bluer towards the central region, indicating the presence of a potentially younger stellar population or ongoing star formation activity in the core. Hints of faint, diffuse extensions surround the main body. There are no clearly defined spiral arms or significant dust lanes visible.
