The galaxy appears as a relatively smooth object, with a slight elongation. It exhibits a prominent central bulge that is bright and concentrated. Extending from the bulge is a faint disk. The disk does not appear to have well-defined spiral arms; instead, it displays some structure indicative of tidal disturbance or interaction with another galaxy. The color gradients suggest that the bulge consists of older stellar populations, while some star formation is present in the disk. There is evidence of a potential merger event, possibly a minor interaction, given the irregular shape of the disk.
