The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical in shape, displaying a high degree of roundness. The central region exhibits a brighter, more intense luminosity, possibly indicating a denser stellar population or active galactic nucleus. The galaxy exhibits a color gradient, with a yellowish hue in the core transitioning to a redder, slightly more diffuse outer region. There is little evidence of distinct spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing a major merger, though a slight visual asymmetry hints at a potential minor gravitational interaction or disturbance. The overall appearance suggests a relatively evolved system, potentially dominated by older stellar populations.
