The galaxy presents as a moderately inclined disk galaxy. A central bulge is visible, appearing largely smooth and dominated by a yellowish-white hue, potentially indicating a population of older stars. Surrounding the bulge is a disk component exhibiting a blueish color, possibly indicative of ongoing or recent star formation activity. The disk appears relatively smooth with some subtle mottling. There is a marginal indication of spiral arm structure. The galaxy appears to be relatively undisturbed, showing no strong signs of a major merger, though there is a hint of a minor interaction or disturbance. Overall, it is a galaxy of intermediate mass, with a low to moderate rate of star formation.
