This galaxy appears to be a relatively smooth, single component system. It exhibits a nearly circular morphology with a slightly elliptical, but not elongated, shape. The galaxy's color profile suggests a dominant older stellar population, with a yellow hue indicating a lower rate of current star formation activity. There is a faint hint of a diffuse, extended halo or envelope surrounding the main body of the galaxy, but no readily discernible spiral arms or prominent dust lanes are observed. There is no strong evidence of any major ongoing merger events or tidal disturbances that could be inferred from the image.
