The galaxy presents as an elliptical or lenticular type, characterized by a smooth, concentrated central bulge. The light distribution suggests a fairly uniform stellar population throughout, lacking prominent spiral arms or distinct dust lanes. A slight elongation is visible, though the overall form appears relatively rounded. Color gradients are subtle, with a tendency toward yellower hues in the central region, indicating an older stellar population. No signs of active galactic nuclei or significant starburst activity are immediately apparent from the broadband imaging. There is no visible evidence of interaction or recent merger events, and the galaxy appears relatively undisturbed.
