The galaxy presents as a relatively smooth and centrally concentrated system. It exhibits an elliptical morphology with a noticeable flattening. The major axis is oriented approximately northeast to southwest. The central region displays a bright, yellowish-white core, potentially indicative of an older stellar population or an active galactic nucleus. Surrounding the core, there's a more diffuse, blueish halo that extends outwards. There is no clear evidence of spiral arm structure or significant dust lanes. The overall color gradient suggests a possible decline in star formation activity from the core outwards. There might be some minor asymmetry in the outer regions, but no major disturbances such as tidal tails or close companions are immediately apparent. The galaxy appears to be relatively isolated and unperturbed.
