The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting a concentration of older stellar populations. Surrounding the core, a more diffuse, blueish halo is visible, potentially indicative of younger, hotter stars and regions of ongoing star formation. The galaxy appears largely spheroidal in shape, with no obvious spiral arm structures or significant dust lanes. There is a slight irregularity, potentially a minor disturbance from a past interaction, but no signs of a major merger event are apparent. Overall, this galaxy appears to be an elliptical or lenticular system, with a relatively substantial stellar mass and moderate levels of star formation activity in its outer regions.
