The galaxy presents as an elongated, cigar-shaped structure, exhibiting a smooth appearance. There is a central, brighter region, perhaps indicating a concentration of older stellar populations. The galaxy displays a color gradient, shifting from a slightly bluer hue towards the outer edges to a redder core, suggesting potential variations in stellar age and composition across the galactic structure. There are no visible spiral arms or strong signs of active star formation regions. The overall morphology appears relatively undisturbed, without evidence of recent major mergers or significant tidal interactions.
