The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The light profile suggests an older stellar population, with a color gradient indicating a higher concentration of older, redder stars toward the galactic center. The overall shape deviates from a perfect circle, exhibiting an elongated, cigar-like morphology. There are no prominent signs of spiral arms or significant dust lanes visible in this image. It appears relatively undisturbed, showing no obvious signs of ongoing major mergers or tidal interactions with other galaxies. Overall, the galaxy appears to be a quiescent system with limited ongoing star formation.
