The galaxy presents as a relatively smooth structure, exhibiting characteristics of an early-type spiral or lenticular galaxy. The central bulge is prominent and appears somewhat elongated. There is evidence of a disk component, viewed at an angle. Patchy regions with a bluish tinge suggest localized star formation within the disk, although this activity is not widespread. The galaxy is relatively isolated, with no obvious signs of ongoing major mergers, though subtle distortions may suggest minor tidal interactions. Overall the galaxy appears to be mature, with a dominant old stellar population and a low rate of star formation.
