The galaxy presents as a flattened, disk-like structure oriented edge-on relative to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, potentially indicative of an older stellar population. The disk is faintly visible and has a bluish tinge, suggesting the presence of younger stars and ongoing star formation. There appears to be a faint dust lane obscuring the central bulge. No significant tidal features or signs of a recent major merger are discernible. There may be a small disturbance visible on the disk in the form of asymmetrical light, which could indicate a minor interaction. The galaxy appears relatively isolated.
