The galaxy presents an elongated, cigar-like morphology. It appears relatively smooth, with a dominant central bulge that exhibits a reddish hue, possibly indicating an older stellar population. Surrounding the bulge, a greenish halo suggests the presence of more recent star formation, potentially fueled by gas and dust. Overall, the galaxy does not appear to be significantly disturbed, displaying a fairly regular structure with no prominent tidal features or signs of major mergers, though some minor disturbance cannot be ruled out. The estimated diameter is approximately 4 kpc. The estimated redshift places it at a distance suggesting it is a moderate sized galaxy. 
