The galaxy presents as a somewhat smooth, elliptical-like structure, with a dominant central bulge. The overall color profile appears slightly redder, suggesting an older stellar population. The galaxy exhibits a moderate level of compactness. No prominent spiral arm structures are discernible, indicating a possible lack of ongoing, large-scale star formation within the disk. The shape is slightly elongated, but mostly circular. There is no apparent merger or tidal disturbance visible.
