The galaxy presents a largely smooth morphology, with a slightly elongated, elliptical shape. Its core exhibits a concentrated brightness, suggesting a higher density of stars in the central region. The light is mostly in a redder spectrum, consistent with a population of older stars. Fainter blueish hues can be seen on the edges, which could indicate a small amount of on-going star formation. Overall, this galaxy appears to be relatively undisturbed, with no strong signs of recent major mergers or tidal distortions.
