The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centrally concentrated structure. The light distribution suggests a relatively uniform stellar population with a slight color gradient. The central region displays a distinct reddish hue, potentially indicating an older stellar population or significant dust obscuration. The outer regions transition to a bluer color, possibly suggestive of more recent star formation or a different population of stars. There's a slight asymmetry or minor disturbance observable in the galaxy's morphology, which could suggest a past or ongoing interaction or merger event. No distinct spiral arms or prominent dust lanes are visible.
