The galaxy appears to be a luminous object with a relatively smooth and concentrated morphology. Its shape is generally round, exhibiting a slight ellipticity. The color profile suggests a dominant population of older stars, giving it a yellowish to reddish hue. There is no clear evidence of spiral arms or a prominent disk structure; rather, the light is distributed more uniformly throughout the galaxy's body. Faint, subtle irregularities are potentially present, hinting at minor past interactions or internal disturbances, but the overall impression is of a well-mixed stellar population in a relatively relaxed dynamical state. The brightness indicates the galaxy is a fairly massive system.
