The galaxy presents as a moderately luminous, early-type system, likely an elliptical or lenticular galaxy given its smooth and concentrated light profile. It exhibits an oblong morphology, being neither perfectly round nor highly elongated, showing a slight cigar shape. The central bulge appears prominent and concentrated. The color indices suggest a relatively old stellar population. There is no apparent sign of recent or ongoing major mergers or strong tidal disturbances. The integrated light appears yellow to orange in color, indicative of evolved stars. There is a low probability of a recent star formation episode. There is no obvious evidence of spiral arms or a prominent disk structure.
