The galaxy presents a generally smooth morphology, with a slightly elongated, elliptical shape. The central region exhibits a concentrated, bright core, suggestive of a significant stellar population density, potentially indicating a supermassive black hole at the galactic nucleus. A subtle color gradient is observed, transitioning from a yellowish-white center to a slightly bluer outer region. This could indicate a younger stellar population in the outer disk relative to the core. There is no evidence of spiral arms or prominent dust lanes. The overall appearance suggests that this galaxy is most likely an early-type galaxy, potentially an elliptical or lenticular galaxy. There are no clear signs of ongoing major mergers or significant tidal disturbances in the image, though subtle asymmetries cannot be ruled out.
