The galaxy presents as a centrally concentrated object with an overall smooth morphology. Its shape is somewhat elongated, appearing cigar-shaped rather than perfectly spherical. The light profile suggests a dominant bulge component, possibly indicating an elliptical classification or a lenticular galaxy seen at an angle. There is no visible dust lane or spiral arm structure to discern, which supports the notion of an older stellar population.

The central region exhibits a distinct reddish hue, which could be indicative of older, cooler stars. The outer regions show a gradual fading of luminosity, with a slight shift towards bluer colors compared to the core, potentially arising from younger stellar populations in the outskirts. There are no signs of significant tidal disturbances or ongoing major mergers.
