The galaxy presents a primarily smooth morphology. It is generally round in shape, with little deviation from a circular appearance. There are suggestions of some minor disturbances in the galaxy's structure, but these are not pronounced enough to categorize it as a major merging event. The galaxy's light profile indicates a concentration of older stellar populations dominating the overall light output, contributing to a redder color. There is evidence of ongoing star formation, but it appears to be at a moderate to low level.
