The observed galaxy presents an elongated morphology, appearing cigar-shaped. The central region exhibits a concentrated luminosity, with the brightest region being in the center. This region transitions into a yellowish color, possibly indicating an older stellar population. Extending from this brighter area, there's a less luminous, diffuse tail-like feature characterized by a bluer hue, suggesting the presence of younger, hotter stars. This extended feature deviates significantly from a smooth elliptical profile, displaying signs of possible tidal distortion or interaction with another galaxy. There is no clear disk-like structure or spiral arm morphology visible. The galaxy's overall appearance suggests a system undergoing some form of interaction or disturbance, affecting its morphology and stellar distribution.
