The galaxy presents as a generally smooth and rounded object. The central region exhibits a concentrated brightness, appearing a warm yellow-orange hue, suggesting an older stellar population or dust obscuration. The outer regions of the galaxy display a gradual decline in luminosity, with a subtle blue-green tint noticeable especially on the edges. This could indicate the presence of younger, hotter stars, or regions of ongoing star formation. The galaxy appears largely undisturbed, without any obvious signs of major mergers or tidal distortions. There might be minor disturbances but they are not apparent in this image. The shape is generally elliptical or possibly a very tightly wound spiral, but the limited resolution makes it difficult to determine the precise morphological type.
