The galaxy presents as a relatively smooth, centrally concentrated object with a diffuse, extended halo. Its overall morphology appears elliptical or lenticular, exhibiting a gradual decrease in luminosity from the core to the outer regions. The core region is characterized by a bright, blueish light, suggesting the presence of a moderate population of young, hot stars or an active galactic nucleus. There is no clear evidence of spiral arm structure or significant dust lanes. Minor morphological disturbance is apparent, potentially indicating a past or ongoing minor merger event. The galaxy appears roughly round in shape, with a faint reddish tinge in the outskirts.
