This galaxy exhibits a defined spiral structure, with discernible arms emanating from a bright, concentrated central bulge. The bulge appears largely smooth and homogenous, suggesting a higher concentration of older stellar populations. The spiral arms display a clumpy morphology, punctuated by regions of intense blue coloration which likely indicates active star formation regions. The arms are not tightly wound, possessing a more open and diffuse appearance. There is some asymmetry to the arm structure with one arm appearing more disrupted, possibly indicating a past interaction. The galaxy's overall shape is elliptical. The galaxy exhibits no obvious signs of a major ongoing merger, but there may be a minor disturbance. There also appears to be a smaller satellite galaxy nearby which may be interacting. The estimated size of the galaxy is a few kiloparsecs across.
