The galaxy presents as a single, relatively smooth, and somewhat compact object. Its overall shape approximates a flattened spheroid, appearing mostly round. The color profile suggests a greater concentration of older stellar populations, indicated by the reddish-yellow hue dominating its central regions, which gradually fades towards the periphery. There is no discernible spiral structure or prominent dust lanes. Subtle variations in color and luminosity suggest a slightly inhomogeneous distribution of star formation.
