The galaxy presents as an elongated, spindle-shaped structure. Its light profile suggests a central bulge that is slightly brighter and more concentrated than the surrounding region. The color of the central bulge appears to be slightly redder, indicating an older stellar population. Moving outward from the center, the galaxy shows a gradual decline in brightness. The outer regions exhibit a bluer hue, suggestive of younger, hotter stars or ongoing star formation, although this activity appears to be relatively low. The galaxy exhibits a generally smooth texture, with no prominent spiral arms or significant dust lanes visible in this image. There is a very slight indication of minor disturbances, but no major merger event or tidal tails are observed.
