The galaxy presents as a moderately bright, disk-shaped structure, exhibiting a notable degree of smoothness in its overall appearance. It appears to be an elliptical galaxy. The galaxy displays a slightly elongated morphology, deviating from a perfectly circular shape. While there are no immediately apparent signs of a major ongoing merger, there are hints of minor disturbances and irregularities. No strong spiral arm structures are readily discernible, but faint disk-like structures are subtly evident. The colour distribution across the galaxy suggests a dominant population of older stars, contributing to its yellowish hue. There is also some evidence of a subtle colour gradient, potentially indicating varying stellar populations.