The galaxy appears as a centrally concentrated spheroid, exhibiting a smooth morphology with no immediately obvious spiral arm structures or significant dust lanes. The color profile suggests a dominant population of older stars, trending towards yellow and red hues in the central region, and fading to a slightly bluer periphery. The shape approximates a circular form with a high degree of roundness, with a slight indication that it may be a disk galaxy viewed face-on. There is no strong evidence of ongoing major merger events or tidal distortions that could disrupt its overall smooth appearance, though a minor disturbance could be present. Overall, it resembles an elliptical galaxy or a lenticular galaxy with little active star formation.
