The galaxy presents as a centrally concentrated system with a smooth, diffuse appearance. Its light profile suggests an elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a slightly elongated shape, deviating marginally from a perfect circular form. There is no clear evidence of major tidal disturbances or ongoing mergers, although subtle asymmetry could indicate minor gravitational interactions in its past. The color distribution indicates that this galaxy is likely populated by an older stellar population.
