The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a smooth, concentrated central bulge. The light distribution is centrally concentrated with an elliptical morphology, with no obvious spiral arm structures or dust lanes visible. The overall color is slightly redder, indicating a stellar population dominated by older, evolved stars. A subtle hint of blue is present in the outer regions of the disk, which may be due to recent or ongoing low-level star formation. The galaxy appears generally undisturbed, with no signs of major mergers or tidal distortions.
