The galaxy presents as a relatively smooth and elongated structure. The color profile suggests an older stellar population, with a dominant yellowish hue concentrated towards the central region of the galaxy. There is a slight gradient in color, with the outermost edges appearing marginally bluer, suggesting the presence of a younger, albeit subdued, stellar population in the galactic periphery. No prominent spiral arms or significant dust lanes are discernible. The morphology leans towards an elliptical or lenticular galaxy type. There is a subtle distortion visible, potentially indicative of a minor gravitational interaction, though the galaxy appears largely undisturbed.
