The galaxy presents as an elongated, disk-like structure, likely a spiral or lenticular galaxy viewed at an oblique angle. The central region exhibits a bright, concentrated bulge, suggesting a significant concentration of stars. The galaxy displays a generally smooth appearance, with a notable lack of distinct spiral arms. The colour gradient shifts from a yellow-white core to a dimmer, slightly bluer periphery. This color gradient indicates a decrease in the population of older stars towards the outer regions. There is an absence of apparent major disturbances or merger activity, and any irregularities seem small and limited in scale. The morphological features and color suggest that this is a galaxy with intermediate to high stellar mass and fairly low star formation.
