The galaxy appears to be an elongated, cigar-shaped system, with a smooth, concentrated central bulge. The color distribution exhibits a gradient, with a yellowish-white core that transitions to bluer hues in the outer regions. There is a suggestion of a faint, extended disk or halo surrounding the main body of the galaxy. There is no obvious presence of spiral arms or significant dust lanes. The overall morphology suggests a relatively evolved system, possibly with ongoing or recent star formation in its outskirts. There is no distinct signs of tidal disturbances or ongoing merger activity.
