The galaxy appears as a concentrated, centrally brightened object with a generally smooth profile. Its overall shape is somewhat elliptical, though nearly circular. There are some subtle color gradients visible, with the central region exhibiting a slightly yellower hue compared to the outer edges which appear more red. The galaxy displays no obvious spiral arm structures or prominent dust lanes. There is no strong evidence of any ongoing major merger events or significant tidal disturbances in the immediate vicinity of the galaxy. The absence of bright blue regions suggest that star formation rates may be relatively low. Overall, the morphology suggests an evolved system.
