The galaxy presents as a somewhat elliptical structure with a relatively smooth, diffuse light distribution. Its color profile indicates a bias towards shorter wavelengths, with a distinct bluish hue, suggesting a relatively younger stellar population. The galaxy shows some subtle internal structural variation, with a slightly brighter, more concentrated central region possibly indicating a galactic bulge. There is no obvious spiral arm structure visible in this image. A slight elongation is apparent, and based on this, the object may have a minor degree of flattening.
