This galaxy presents an elongated, cigar-shaped morphology. The color profile indicates a predominantly older stellar population, with a concentration of yellow and redder hues in the central region. The light is smoother and more diffuse than irregular. Hints of a possible disk structure are present, though not sharply defined. No strong tidal features or other signs of recent major merger events are visible. There are no regions of concentrated blue light, which is characteristic of higher star formation. Small distortions might be present, indicating minor disturbances, though the general structure appears relatively undisturbed.
