The galaxy presents a somewhat smooth morphology. It appears elongated, with a high degree of asymmetry. The central region exhibits a brighter, more concentrated luminosity profile, possibly indicating a substantial stellar population. The overall color suggests a range of stellar ages, with a dominant presence of older, redder stars. There is faint evidence of a possible minor disturbance in the galaxy's shape or structure, though the main body appears relatively undisturbed. The galaxy does not appear to be actively merging with another galaxy. A hint of bluer light in some spots could suggest modest levels of star formation.
