The galaxy presents as a lenticular or possibly an elliptical type system. The central bulge is prominent and exhibits a smooth, yellowish-orange color, suggesting a relatively old stellar population dominated by red giant stars. The light is highly concentrated towards the core, indicating a high density of stars within the bulge. A faint, elongated disk or halo surrounds the central bulge. It is difficult to discern distinct spiral arm structures, if any are present. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or mergers with other galaxies. There is little to no evidence of active star formation.
