This galaxy presents as an edge-on spiral or lenticular galaxy. The central bulge is prominent and exhibits a yellowish-white hue, suggesting a population of older stars. The disk component appears relatively smooth and elongated, with some faint blueish regions at the extremities, which might indicate areas of recent or ongoing star formation, albeit at a low rate. There are no obvious signs of strong dust lanes or tidal disturbances. The overall morphology suggests a galaxy that is not actively undergoing a major merger, but slight asymmetries may indicate minor gravitational interactions. The galaxy's apparent size is relatively compact and its luminosity is high.
