The galaxy appears to be a relatively smooth, early-type spiral or lenticular galaxy. Its overall shape is elliptical, tending toward round, with a central bulge region that dominates the galaxy's luminosity. The bulge exhibits a yellowish-white color, indicative of an older stellar population. Moving outward from the core, a disk structure can be faintly observed. There is little evidence of distinct spiral arms, but there are some slight blueish tinges that suggest small amounts of recent star formation. No significant dust lanes or active star-forming regions are immediately apparent. The galaxy appears to be relatively isolated, showing no major signs of ongoing or recent mergers.
