The galaxy presents a generally smooth morphology. It appears largely elliptical, with an intermediate axial ratio, not deviating significantly from a circular shape. The color gradient suggests a central concentration of older stellar populations, indicated by the slightly redder hue in the core. The outer regions exhibit a bluer color, indicative of younger stars or ongoing star formation, but this activity appears relatively subdued. There is no obvious evidence of spiral arms, strong dust lanes, or significant tidal disturbances suggesting major merger events. The galaxy exhibits a relatively symmetrical profile.
