This galaxy presents as a relatively small, elongated lenticular or edge-on spiral, likely at an intermediate redshift. Its overall structure appears smooth, with a bulge-dominated morphology lacking prominent spiral arms. The central bulge exhibits a slightly brighter, more concentrated luminosity profile, surrounded by a fainter, extended disk. The color gradient suggests subtle variations in stellar populations or dust content across the galaxy. The observed colors indicate ongoing, but relatively low levels of star formation, contributing to a bluish tinge within the disk, though older stellar populations are still prevalent. There is no apparent evidence of major mergers or significant tidal disturbances in the immediate vicinity, suggesting a relatively isolated evolution, but minor interactions cannot be ruled out given the potential for subtle morphological irregularities within the disk.
