The galaxy presents as a somewhat centrally condensed object with a diffuse, albeit faint, extended halo. The core region displays a smooth, almost amorphous structure, with a slight elongation visible in the north-south axis. While the galaxy generally lacks sharp, well-defined spiral arms, there are subtle variations in the light distribution suggestive of possible faint, diffuse features extending outwards from the central region.

A slight hint of disturbance is apparent, possibly indicative of a minor interaction. The overall shape is tending towards round, without being completely circular; with a hint of a cigar shape.

The galaxy exhibits a relatively blue color profile in its central and near-central regions, gradually diminishing with redshift. The outer halo appears comparatively redder, though this could be influenced by the limited color information available in the z-band. It is hard to confidently determine if the redder hue is a result of a strong presence of dust and/or older stellar populations.
