The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, elongated with a cigar-like form. A prominent bulge is visible, exhibiting a yellowish-orange color, suggesting an older stellar population dominating the galaxy's core. The outer regions appear fainter with a subtle blue tinge, potentially indicating the presence of some younger, hotter stars or ongoing star formation at a low rate. There are no clear signs of spiral arms or significant dust lanes. The overall structure suggests that the galaxy has likely undergone significant morphological evolution, possibly through mergers or interactions with other galaxies, although no major disturbances or ongoing mergers are evident in the image. The lack of distinct features and smooth appearance points towards it being a relatively evolved system.
