The galaxy presents as a relatively smooth, elliptical morphology. There is a concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. Fainter, bluer emissions are visible towards the outer regions of the galaxy, possibly indicating ongoing, though low, star formation. The galaxy is moderately elongated and appears relatively isolated with no obvious signs of major mergers or strong tidal disturbances. The overall appearance suggests a galaxy that is somewhere between an elliptical and a lenticular galaxy, with a dominant spheroidal component.
