The galaxy presents as a roughly elliptical structure, though with a slight elongation suggestive of a mild disk component. The central bulge is prominent and exhibits a smooth, concentrated light distribution, appearing yellowish, which may indicate an older stellar population. The outer regions show a fainter, bluer hue, implying some ongoing star formation activity, albeit at a low level. There are no obvious signs of spiral arms or significant morphological disturbances. The galaxy appears relatively isolated, without any clear indications of recent major merger events, although minor tidal features cannot be entirely ruled out given the image resolution. Overall, the galaxy appears to be an intermediate stage between a spiral and elliptical type, potentially evolving into a lenticular galaxy.
