The galaxy presents a generally smooth appearance, with a subtle elongation in its overall form. The central region appears brighter and more concentrated, suggesting a higher density of stars or other luminous material. Faint, diffuse light extends outwards from the core. The color profile indicates the presence of relatively young, star-forming regions, or potentially an active galactic nucleus with emission lines contributing to the observed bluer hues. Overall, the galaxy appears relatively undisturbed, lacking strong indications of recent major merger events.
