The galaxy presents an overall smooth morphology with a relatively high degree of central concentration. It exhibits an elliptical shape, appearing significantly elongated along one axis. A discernible bulge component is observed in the galaxy's core, characterized by a yellowish hue, indicative of an older stellar population. The outer regions appear bluer, suggesting the presence of younger stars and ongoing star formation, albeit at a modest rate. There is no visible evidence of spiral arm structure or bar features. The galaxy shows no significant signs of tidal interactions or major disturbances, although a minor irregularity in the outer halo cannot be ruled out.
