The galaxy presents as a relatively compact, early-type system. Its morphology appears smooth and elliptical in shape, exhibiting a high degree of central concentration with no discernible spiral arm structure. The galaxy displays a yellowish-orange hue, suggesting an older stellar population with diminished recent star formation. There are no obvious signs of significant tidal disturbances or ongoing mergers. It is an isolated system. The galaxy appears to be relatively massive and luminous, with a quiescent star formation rate.
