The galaxy presents a somewhat elongated morphology, appearing more cigar-shaped than round. The light distribution suggests a predominantly smooth structure, although hints of internal features are visible. There may be a subtle disk-like structure within the central region. The color gradients indicate the possible presence of both older stellar populations, emitting in the redder wavelengths, and areas of more active star formation, apparent as blue regions, scattered throughout the galaxy. There are signs of disturbance in the galaxy's overall structure, potentially indicative of minor gravitational interactions or ongoing merger activity. The relatively high star formation rate suggests the galaxy is actively building its stellar mass.
