The galaxy presents as an elongated, moderately luminous object. It appears to have a relatively smooth morphology, lacking the distinct spiral arm structures or irregular features typically associated with ongoing major mergers. The light distribution is concentrated towards the center, suggesting the presence of a significant bulge component. The overall color profile indicates a mixture of stellar populations, with a noticeable presence of older, redder stars. However, there is also some suggestion of bluer, potentially younger stars intermixed in parts of the galaxy. There is a mild tidal distortion present, which may mean there is minor merger activity. The object appears to be experiencing moderate star formation, with an overall stellar mass that is significant.
