The galaxy exhibits an elongated morphology. The central region presents a high surface brightness, appearing largely smooth and concentrated, with a yellowish hue, suggestive of an older stellar population. Extending from one side of this central bulge is a fainter, bluish extension or tidal tail, indicating ongoing or recent gravitational interaction. The galaxy does not possess well-defined spiral arms. There is some indication of asymmetry in the overall structure, possibly indicative of a minor disturbance or an early stage merger event. Overall, the galaxy appears to be in a state of flux, either settling into a stable form or experiencing external influence.
