This galaxy presents an elongated, cigar-shaped morphology. Its central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population and potentially a lower rate of current star formation activity in the core region. The galaxy lacks defined spiral arm structures, indicating it is likely a lenticular or early-type spiral. The outer regions of the galaxy display a gradual decrease in luminosity, blending smoothly into the background. There appears to be some degree of asymmetry, but it is difficult to tell if it is the beginning stages of a merger. The estimated mass appears to be quite significant.
