The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a smooth, centrally concentrated morphology with a lack of well-defined spiral arms. The galaxy's color profile suggests an older stellar population, with a dominant yellowish-orange hue at the core, gradually fading towards the outer regions. The light distribution indicates a centrally dominant spheroid with a relatively high degree of rotational symmetry, lacking prominent features such as dust lanes or active star-forming regions. There is a very subtle flattening in the disk indicating it's transitioning into a spiral. It may possibly be undergoing minor disturbances due to a possible merger in its past.