The galaxy presents as an elongated, cigar-shaped structure. It appears relatively smooth in texture, with a dominant central bulge that is somewhat indistinct and diffused. There is evidence of a disk component, although it is not clearly resolved. The color gradient shows a bluer hue on one side of the disk, likely indicating regions of active star formation. The opposite side of the disk exhibits a reddish tint, possibly indicative of an older stellar population or dust obscuration. There is no obvious indication of a major ongoing merger, although subtle irregularities could suggest minor gravitational interaction or disturbance. Overall, the galaxy seems to be a relatively quiescent system, with a moderate degree of star formation.
