The galaxy presents a primarily elliptical morphology, appearing largely smooth and relatively featureless in this image. There's a concentration of light towards the central region, suggesting a prominent galactic nucleus. The light is concentrated, but quickly disperses. The galaxy appears to have an intermediate axial ratio, appearing as a relatively smooth, elongated structure rather than a perfect circle. There is a slightly redder hue which could indicate an older stellar population. No significant signs of tidal disturbances or ongoing major mergers are apparent in this image, though there might be minor asymmetries that are hard to interpret.
