The galaxy presents a generally smooth morphology. A bright central bulge, exhibiting a yellowish hue, dominates its structure. The galaxy appears relatively round in shape, suggesting a classification towards elliptical. There is a subtle hint of asymmetry in the outer regions. Furthermore, there is a possible tidal tail or plume visible extending slightly from the main body, which suggests a minor gravitational interaction or past merger event. The redder color suggests older stellar populations. There may be some dust obscuring the central bulge. The galaxy has a definite bulge with little to no visible spiral arms. It displays no strong evidence of active star formation, but this should be tested with more sensitive observations. 
