The galaxy appears to be a relatively smooth, elongated system. Its shape resembles a flattened spheroid, possibly indicative of an elliptical galaxy viewed at an oblique angle or a lenticular galaxy. The central region exhibits a brighter, more concentrated light distribution, suggesting a bulge component. There is a subtle color gradient, with the core appearing slightly more yellow/orange compared to the bluer hues observed in the outer regions. There are no clear signs of spiral arms or significant dust lanes. There are no obvious signs of tidal disturbances or ongoing major mergers, although subtle asymmetries or minor disturbances cannot be ruled out. It has a relatively low star-formation rate.
