The galaxy presents as a somewhat elongated, elliptical form. It exhibits a relatively smooth morphology, with no immediately apparent spiral arms or significant dust lanes. The central region appears brighter and more concentrated, indicating a possible bulge component. The color gradient transitions from a yellowish core, suggestive of an older stellar population, to a bluer periphery, hinting at the presence of younger, hotter stars and ongoing star formation activity, especially in the galactic disk. The galaxy appears relatively isolated, showing no signs of recent or ongoing major merging activity or strong tidal disturbances. It's overall shape is cigar-like.
