The galaxy appears as a smooth, elliptical structure with a concentrated central bulge. The light distribution is relatively even, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The galaxy appears to be somewhat elongated, leaning closer to an "in between" shape than perfectly round. The core exhibits a yellowish hue, which likely indicates an older stellar population. The outer regions appear somewhat bluer, suggesting the presence of some younger stars or ongoing star formation, albeit at a low rate. There are no obvious signs of a major merger or tidal disturbance. A faint, subtle asymmetry exists in the outer regions, indicating possible minor interactions.
