The galaxy presents as a somewhat smooth, disk-like structure with a distinct central bulge. The overall shape is elliptical, appearing elongated along a single axis. The bulge exhibits a yellowish hue, suggesting an older stellar population. The disk component displays a gradient in color, with a blue-green tint visible outside the bulge and along the outer edges, potentially indicating the presence of younger, hotter stars and ongoing star formation. There are no obvious signs of a major merger event, however a small irregularity is apparent on the left side, possibly a minor disturbance.
