The galaxy exhibits a relatively smooth morphology with an elliptical shape, appearing elongated along its major axis. The central bulge is prominent and displays a yellowish hue, suggesting a population of older stars. The outer regions show a gradual fading in luminosity, and present a bluer color. This color likely indicates more recent star formation activity in the outer disk relative to the galactic bulge. There are no immediately obvious signs of spiral arm structure or major disturbances in the galaxy's overall form, though the elongation could possibly be signs of a minor disturbance. The observed galaxy shows a quiescent state, with an older stellar population.
