The galaxy appears as a relatively small, faint, and somewhat elongated object. Its overall structure suggests a disk galaxy viewed at an oblique angle. The light distribution is concentrated towards the central region, indicating a possible bulge. The disk component appears relatively smooth with no strong evidence of distinct spiral arm structures. There are hints of subtle variations in color across the galaxy, with a slightly bluer hue visible, possibly indicating regions of more recent star formation. No apparent distortions or tidal features are visible, suggesting the system has not experienced major recent interactions, although some minor disturbances cannot be ruled out. The galaxy exhibits no distinct features of an active galactic nucleus.
