The galaxy presents as a cigar-shaped, smooth structure. It displays a dominant, relatively uniform bluish color gradient, indicative of a younger stellar population and ongoing star formation. The morphology appears to be that of an elliptical galaxy, elongated in shape. There is an apparent absence of prominent spiral arms or a well-defined disk.

The light distribution is centralized, suggesting a concentration of stars toward the galactic core. No significant dust lanes or obscuring material are readily apparent in this image. The overall appearance suggests a relatively evolved system with a generally homogeneous stellar population. However, the color indicates that there is still some ongoing star formation, which could be due to a recent minor merger. Overall, the galaxy seems to have a mass of around 10^9.5 solar masses. 
