The galaxy presents a generally smooth morphology. The light distribution suggests an elongated shape, with a clear major axis. There is a slight indication of disturbed morphology, potentially from tidal interactions or a recent minor merger event. There appears to be a separate region of star formation detached from the main body of the galaxy.
The color gradient transitions from blue-ish hues at the edges to redder colors at the center. This color gradient suggests ongoing star formation in the outer regions, and an older stellar population in the central bulge. The galaxy appears to be relatively low-mass, given its overall size and luminosity.
