The galaxy presents as a generally smooth, elliptical morphology with a concentrated central bulge. It exhibits a nearly circular form, with only very slight elongation. There is a smooth transition from the bright central region outward, with no distinct spiral arms or other prominent features. A subtle color gradient is discernible, with the core appearing slightly bluer than the outer regions, suggesting a moderate level of recent star formation. The galaxy does not appear to be undergoing any major mergers or tidal disturbances. Overall, the structure indicates a relatively evolved system, possibly a lenticular galaxy, with diminished current star formation.
