The galaxy presents as an elongated spheroid, exhibiting a moderately smooth texture across its visible structure. A discernible color gradient exists, transitioning from a bluish hue at the galactic periphery to a warmer, yellowish tone toward the core. The outer regions of the galaxy, while somewhat indistinct, appear to lack well-defined spiral arm structures, suggesting a morphology more closely aligned with lenticular or early-type spiral classification. The galaxy displays a degree of internal activity, with notable star formation occurring within its disk, and the core is indicative of an older stellar population. Overall, the galaxy's morphology suggests a system undergoing a transition phase in its evolution.
