The galaxy presents as a relatively smooth, elliptical or lenticular morphology, exhibiting a concentrated central bulge. Color gradients suggest a subtle variation in stellar populations; the central region appears yellowish, potentially indicating older, redder stars. A faint, blueish haze surrounds the core, which may be indicative of a small amount of on-going star formation. The overall structure does not show signs of major disturbances or tidal features. The galaxy exhibits a high degree of circular symmetry.
