This galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated structure with an approximate diameter of 3 kpc based on estimated values. The color distribution indicates an older stellar population, concentrated towards the galactic center, with a slight shift towards blue hues in the outer regions, possibly suggesting regions of more recent though modest star formation. The galaxy appears somewhat elongated. There is no obvious evidence of strong tidal interactions, but slight distortions could suggest minor disturbances. No prominent spiral arm structures or a well-defined disk are apparent. The galaxy is not perfectly spherical, appearing more as a spheroid.
