The galaxy presents a generally smooth, elliptical morphology, characterized by a high degree of central concentration. The light profile appears regular, without prominent spiral arms or bar-like features. The core exhibits a yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation. Moving outward from the core, the galaxy gradually fades into a fainter halo. There is no evidence of significant tidal interactions, major disturbances, or a recent merger event. Overall, the galaxy appears well-relaxed, indicating it has likely undergone significant dynamical evolution.
