The galaxy presents as a relatively smooth, disk-like structure, elongated in shape. The central region exhibits a pronounced concentration of light, appearing brighter and slightly redder in color than the surrounding areas, suggesting an older stellar population and/or significant dust obscuration in the core. Extending outward from the central bulge is a fainter disk component, showing some evidence of structure although not highly resolved. This disk appears more bluish-green, potentially indicative of younger, hotter stars and ongoing star formation. There are no obvious signs of a major ongoing merger or strong tidal interactions, though subtle irregularities or minor disturbances in the outer regions cannot be ruled out at this resolution. The overall color profile suggests a galaxy with an intermediate age stellar population.
