The galaxy presents as a slightly elongated, disk-shaped structure, though the bulge to disk ratio is not readily apparent from visual inspection. The central region exhibits a higher surface brightness and a yellow-white hue, suggestive of an older stellar population. Extending outwards from the center, a fainter, bluer disk is visible. This likely indicates ongoing star formation, albeit at a moderate rate. The overall morphology appears relatively undisturbed, showing no clear signs of a recent major merger, but possible minor disturbance with some asymmetries in the outer disk structure. There are no prominent spiral arm structures easily discernible. The galaxy's angular size is modest, consistent with a galaxy at intermediate redshift. The color indices imply a system that is transitioning, with recent to ongoing star formation occurring amidst an older, more passively evolving stellar population.
