The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its shape approximates a rounded form. There is little evidence of distinct spiral arm structure or significant tidal features, suggesting it is not undergoing a major merger or significant gravitational disturbance. The color indices imply the presence of an older stellar population, exhibiting a redder color, with some hints of more recent star formation present. Overall, the galaxy exhibits characteristics consistent with a relatively quiescent state, with minimal ongoing starburst activity.
