The galaxy presents a primarily smooth morphology, with a concentrated central bulge exhibiting a yellowish hue. There is a subtle disk-like component exhibiting a faint bluish tint surrounding the bulge, suggesting the presence of younger stellar populations and some ongoing star formation, although it appears weak. The galaxy exhibits a fairly regular structure without any pronounced signs of tidal disturbances or recent major merger events. Overall the galaxy appears to be an intermediate mass system undergoing moderate star formation.
