The galaxy presents an elongated, cigar-like morphology. The central region exhibits a higher surface brightness and a yellowish-orange hue, suggesting an older stellar population. This region appears relatively smooth, with no prominent dust lanes or spiral arm structures visible. Extending outwards from the central bulge, the galaxy appears to fade gradually, suggesting a declining stellar density. The overall color profile suggests a more evolved system, with a lower rate of ongoing star formation activity. There is a hint of minor disturbance or interaction with a smaller galaxy in the vicinity.