This galaxy presents as a moderately luminous system with an overall elongated morphology, appearing as a disk seen at an oblique angle. The central region exhibits a concentrated bulge, characterized by a yellowish-white hue, suggesting a population of older stars. The surrounding disk shows hints of a spiral structure. On the far side of the disk, blue tinges are visible that likely indicates areas of active star formation, although the overall disk appears relatively smooth, with only subtle variations in color and intensity. The galaxy does not show any major signs of disturbance, such as tidal tails or other indicators of recent major mergers, though there is minor asymmetry that is visible. The object is relatively compact and appears to be a galaxy of intermediate mass.
