The galaxy presents a generally smooth morphology, with a concentrated central region exhibiting a yellowish-white hue, indicative of an older stellar population. The galaxy appears largely elliptical in shape with a high degree of roundness. There is no clear indication of spiral arm structure or significant dust lanes. No major ongoing merger events are visible. Faint blue emission may be present in the outskirts, suggesting some recent or ongoing star formation, albeit at a low rate. Overall, the galaxy's characteristics point towards a relatively evolved system.
