The galaxy presents as a largely featureless, elliptical or lenticular type object. It exhibits a high degree of central concentration, with the light profile appearing smooth and radially symmetric. There's a clear radial color gradient, with the core appearing more yellow, suggesting an older stellar population dominating the central region. The outer regions exhibit a subtle blueish hue, potentially indicating some presence of younger, hotter stars, or perhaps some dust content causing reddening in the interior. There is no visible spiral structure or significant morphological disturbance, such as tidal tails or asymmetric features to suggest recent major merger activity. The galaxy appears well-defined.
