The galaxy presents a predominantly smooth morphology, appearing as an elongated spheroid with a cigar-like shape. A central bulge, characterized by a yellowish-white hue, is visible, suggesting an older stellar population. The galaxy exhibits a disk component, and is also characterized by blue regions that likely indicate the presence of younger, hotter stars, and ongoing star formation. No prominent spiral arm structures or signs of a recent major merger are immediately discernible, however, there may be a small disturbance present. Overall, the galaxy exhibits a relatively quiescent state of evolution.
