The galaxy presents an elongated, cigar-shaped morphology. A pronounced color gradient is observed, with one end exhibiting a distinct reddish hue, transitioning towards a bluer spectral signature across the main body of the galaxy. This color variation suggests spatial differences in stellar populations, dust content, or redshift.

The galaxy's structure appears relatively smooth across its major axis, though there are hints of possible tidal disturbances or minor interactions, particularly at the fainter edges. The disk exhibits a possible bulge on the left side, as indicated by the color and light intensity. Further data is needed to determine the cause of this potential disturbance.

There is no clear spiral arm structure visible within the galaxy at this resolution. The galaxy is most likely an edge-on lenticular galaxy undergoing minor disturbances.
