The galaxy presents as a relatively compact system, appearing as a smooth central bulge with a disk-like extension. The overall shape is elongated, showing a deviation from perfect circular symmetry. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. Extending from the central region is a more diffuse structure with a bluer color, suggesting the presence of younger, hotter stars, or perhaps areas of ongoing star formation. There is a visual asymmetry to the overall galactic structure, potentially due to tidal interactions with another galaxy, though there isn't a visible secondary galaxy in this image. The distribution of light within the galaxy is not uniform, with the central bulge being much brighter than the outer regions.
