The galaxy presents as a relatively compact, disk-shaped system oriented at a significant inclination to our line of sight. There appears to be a clear separation in color, with one end showing a yellowish-white hue, grading into the other with a blue-green tint. The yellowish-white end suggests the presence of an older stellar population, where star formation has largely ceased or is occurring at a reduced rate. Conversely, the blue-green region indicates ongoing star formation, likely hosting younger, hotter stars. The overall morphology lacks strong evidence of spiral arm structures and has a somewhat smooth appearance. There is no strong evidence of a recent major merger, however minor disturbances cannot be ruled out. Overall the galaxy appears to be a late stage disk galaxy.
