This galaxy presents an elongated morphology, appearing as a flattened spheroid with a defined major axis. A pronounced central bulge is visible, exhibiting a yellowish-white hue. There is a distinct disk structure oriented nearly edge-on with respect to our line of sight. The disk appears bluer in color compared to the bulge, potentially indicating more active star formation regions with a higher proportion of young, hot stars. There is a slight asymmetry visible in the disk, with a hint of possible tidal disruption or an interaction with a companion, or even a slight warp. The outer regions of the disk appear fainter, and somewhat mottled. Overall the galaxy presents a relatively smooth appearance, though subtle features suggest it is not a completely undisturbed system. There is potentially some minor disturbance or merger activity that may contribute to the asymmetry, but the general structure remains intact.
