The galaxy presents as a relatively smooth, disk-shaped structure, appearing somewhat elongated. A central bulge is visible, exhibiting a yellow-orange hue, suggesting an older stellar population concentrated in the core. Fainter, bluer regions extend from the bulge into the disk, likely indicating areas of ongoing star formation. There appears to be some minor disturbance in the morphology, perhaps an indication of a past or ongoing minor merger event. Overall, the galaxy appears to be an intermediate stage in its evolution, not a pure elliptical but not a well defined spiral either.
