The galaxy appears as a somewhat elliptical structure, exhibiting a smooth light distribution. There is a distinct central bulge that appears brighter and yellower in color, likely indicative of an older stellar population. The outer regions fade gradually and appear more elongated, suggesting a flattened disk-like component, viewed at an angle. I observe a generally undisturbed morphology with no obvious signs of recent major mergers or tidal interactions. There is a hint of redder color on the edges, which could indicate dust.
