The galaxy presents a generally smooth, elliptical morphology. Its color gradient transitions from a central reddish-orange hue to a more diffuse, greenish-blue outer region. This may indicate a concentration of older stellar populations toward the core, with younger, bluer stars residing in the galaxy's outskirts, though this interpretation is tentative without spectroscopic data. There is no readily apparent spiral structure or distinct dust lanes. The overall shape suggests the galaxy is an elliptical type, possibly of intermediate size based on the color profile. There are no signs of significant tidal distortion or ongoing mergers, the object appears mostly relaxed and undisturbed, with perhaps minor evidence of recent interaction in the outskirts. The galaxy's light profile is concentrated toward the center, consistent with a high degree of central mass concentration.
