The galaxy presents as an elongated, cigar-shaped structure. It appears to be relatively smooth in texture, exhibiting a lack of distinct spiral arms or significant clumps of star formation regions. The color gradient suggests a concentration of older stellar populations. There is a subtle color change from the core outwards, indicating possible radial differences in stellar populations or dust distribution. There is some indication of a possible minor tidal disturbance, but there are no clear signs of a recent or ongoing major merger event. 
