The galaxy presents as a lenticular system, with a dominant bulge and a faint, elongated disk structure. The bulge region exhibits a smooth, concentrated luminosity profile, suggesting a population of older stars. The disk is less defined and shows no prominent spiral arm features. The overall shape is highly elongated, with an axial ratio indicating a significant inclination relative to our line of sight. There is no evidence of major mergers or strong tidal disturbances. The color gradient transitions smoothly from a yellower bulge to a bluer disk, hinting at ongoing, though potentially low, star formation activity in the disk component. The system is relatively isolated.
