The galaxy presents a generally smooth morphology, with a dominant central bulge that appears roughly circular. The light distribution suggests a high degree of central concentration. There may be a faint disk component visible, but its features are not distinct. Some irregularities are visible in the light distribution, possibly indicating minor disturbances within the galaxy, or potentially early stages of a merger with another galaxy, although its smooth shape makes it hard to confirm. The primary color of the galaxy is yellowish, consistent with an older stellar population, although there are bluer regions that may indicate recent star formation.
