The galaxy presents as a relatively smooth, centrally concentrated object. It appears to have a somewhat elliptical morphology, with no apparent spiral arm structures or a prominent disk component visible in this image. The overall color profile suggests a more evolved stellar population. There is a hint of a slight disturbance in the outer regions, but no distinct signs of a major merger or strong tidal interactions. The light distribution is centrally bright and gradually fades out towards the edges. Based on the roundness of the galaxy, the light appears to be between circular and cigar shaped. The galaxy appears to have a very low rate of star formation.
