This galaxy presents as a late-type spiral system observed at an oblique angle, with significant disk inclination relative to our line of sight. The central bulge appears moderately bright and has a yellowish hue, indicative of an older stellar population. Surrounding the bulge is an extended disk, exhibiting bluer colors suggesting ongoing star formation. While detailed spiral arm structure is not easily discernible due to the viewing angle, the disk displays irregular light distribution, potentially revealing the presence of star-forming regions. The dust lanes seem present obscuring parts of the bulge and disk. The apparent magnitude of this galaxy is relatively faint, implying a considerable distance. Considering the overall morphology, this galaxy is likely undergoing active star formation and possesses a moderately substantial stellar mass. There may be some interaction with a small nearby galaxy which could have minor disturbance morphology. 
