The galaxy presents a mostly smooth morphology, with a slight elongation in its overall shape. Its colour profile indicates an older stellar population, dominated by yellowish hues concentrated towards the central bulge, suggesting reduced star formation activity. The presence of bluer colours extending outwards hints at the presence of younger stars in the disc, indicating a more recent period of star formation in the outer regions of the galaxy. There are very minor visual disturbances, so there may have been a small merger in the distant past.
