The galaxy presents as a somewhat smooth, elongated structure. The central bulge region exhibits a bright, concentrated luminosity, suggesting a high density of older stellar populations. Moving outward from the bulge, the galaxy fades into a less defined disk, although some faint disk-like features are present. The galaxy appears to have a slight inclination relative to our line of sight. The overall color is predominantly yellow, indicative of a significant population of evolved stars. There is no strong evidence of recent major merging activity, although there may be some minor disturbance in the outer regions. The galaxy's morphology appears to be somewhere between a lenticular galaxy and an elliptical galaxy. The rate of star formation is estimated to be quite low. The galaxy mass is fairly large.
