The galaxy presents as an edge-on spiral, exhibiting a flattened disk structure. The central bulge is prominent and appears somewhat rounded, gradually fading into the surrounding disk. There are no observable signs of active galactic nuclei activity or a major merger event. The color profile suggests a stellar population with ongoing star formation, based on the blueish tint across the disk, although there is no specific evidence of defined spiral arms. The galaxy’s overall smooth appearance implies it could be a relatively evolved system, with a considerable fraction of its stars residing in the disk component.
