The galaxy appears as a centrally concentrated object with a generally elliptical morphology. Its light profile seems relatively smooth, with no apparent spiral arm structures or distinct morphological features visible in this image. The color is predominantly yellowish-orange, suggesting an older stellar population with lower levels of recent star formation. There are subtle variations in color across the galaxy, but the overall impression is that of a fairly homogenous stellar distribution. The galaxy's central region appears slightly more concentrated and possibly slightly redder than its outer regions. There is no clear evidence of a dust lane or any significant ongoing merger activity based on visual inspection of the galaxy's shape.
