This galaxy presents as an elliptical or lenticular system, exhibiting a relatively smooth and concentrated light profile. There is a noticeable absence of distinct spiral arm structures or prominent dust lanes. The galaxy appears more elongated than perfectly circular, tending toward a slightly flattened shape. Its color suggests a population of older stars, with a yellowish or reddish hue dominating. Any potential central bulge is difficult to resolve with the available data. The galaxy seems to be relatively undisturbed, showing no major signs of ongoing merger activity or significant tidal distortions.
