The galaxy exhibits a somewhat elliptical morphology, with a central bulge that appears relatively smooth and concentrated. There are hints of a disk component, but it is not well-defined, and the galaxy lacks prominent spiral arms. The color of the central bulge is yellowish-white, suggesting an older stellar population. The outer regions of the galaxy appear bluer, which could indicate the presence of younger, hotter stars and ongoing star formation. However, this star formation does not appear highly active. There is evidence of disturbance in its morphology, potentially indicating a past or ongoing interaction with another galaxy. The galaxy's overall appearance suggests it is a galaxy transitioning in type, perhaps from a spiral to an elliptical as it interacts with other galaxies.
