The galaxy presents as a single, dominant spheroidal structure. It appears generally smooth, with a concentrated central bulge that dominates the visual appearance. The galaxy exhibits a color gradient, transitioning from a yellow-orange core to a redder outer halo. There is little evidence of spiral arms or distinct substructure within the galaxy, although subtle irregularities in the light distribution may be present in the outer regions. The overall shape is approximately elliptical, with some deviation from perfect roundness. Indications are that the object is a relatively massive galaxy, with a relatively low star formation rate. The surrounding area shows no significant signs of major gravitational disturbances or ongoing mergers.
