The galaxy presents as a somewhat elongated, disk-shaped object. It exhibits a smooth, relatively featureless morphology, suggesting a lack of prominent spiral arms or significant star-forming regions. The central bulge appears prominent, with a noticeable concentration of light that fades gradually outwards towards the edges of the galaxy. The color profile indicates a reddish hue, possibly due to an older stellar population or significant dust obscuration within the galaxy. There's no clear indication of ongoing major merger activity or tidal disturbances, though subtle irregularities cannot be entirely ruled out given the image quality. It appears to be a relatively undisturbed system.
