The galaxy presents a primarily smooth morphology, appearing largely spheroidal in shape. A concentration of light is observed towards the center with an overall yellowish hue that suggest an older stellar population. The central region appears brighter and more compact. The galaxy lacks any distinct spiral arm features or significant dust lanes. It exhibits a noticeable color gradient, transitioning from a yellowish center to a slightly bluer periphery. There is no evidence of major ongoing merging events or significant tidal disturbances, although there might be a minor disturbance present.
