The galaxy appears as a somewhat elongated structure, with a pronounced cigar-like shape. There is evidence of a prominent smooth component, alongside fainter, more diffuse features. It presents with an observable color gradient. A distinctly yellow region is apparent, while other regions tend toward bluer hues. The galaxy's shape suggests that it is relatively undisturbed, and that is not undergoing any kind of significant merger. However, there may be some minor disturbance, perhaps indicating a slight interaction. The overall luminosity is relatively low, indicating a lower stellar mass and a relatively low rate of star formation.
