The galaxy presents as a spiral type, exhibiting a prominent central bulge that appears to be a significant fraction of the galaxy's overall light output. The bulge is circular and smoothly concentrated. The disk is inclined to our line of sight. Spiral arms are visible and are moderately wound, presenting a fairly clear structure. The galaxy shows a subtle asymmetry indicative of either tidal interactions or an ongoing minor merger event. The color distribution suggests a mix of stellar populations, with the bulge appearing redder and the disk showing bluer regions, especially along the spiral arms, possibly indicating areas of active star formation. The galaxy’s overall shape is elliptical. Dust lanes appear subtle within the spiral arms but are not dramatically obscuring the light.
