The galaxy presents as a moderately luminous, relatively compact object. Its morphology appears predominantly smooth and elliptical, exhibiting a high degree of roundness. A central bulge region is visible with a concentration of light, suggesting a significant population of older stars. The outer regions display a slightly bluer hue, possibly indicative of some ongoing star formation, although this is not a dominant characteristic. There is no obvious evidence of a spiral structure or major disturbances due to mergers, though subtle asymmetries in the light distribution might suggest minor interactions or internal dynamic processes. The galaxy does not show any obvious signs of a dust lane. 
