The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in intensity outward from the core. The galaxy has a slightly flattened shape, deviating from a perfect sphere. There is little to no evidence of spiral arms or a prominent disk structure. Its color suggests a relatively older stellar population, with a subtle blue hue indicating ongoing or recent star formation. No major disturbances or signs of an ongoing merger are visibly apparent. The galaxy is a relatively medium sized.
