The galaxy presents a generally smooth appearance, although a slight irregularity can be noted. Its overall morphology is that of an elongated, cigar-shaped structure. The central region of the galaxy exhibits a brighter, more concentrated luminosity. There is evidence of a disk structure, as indicated by a slight flattening along its primary axis. There are no obvious signs of recent major merger events. There may be some minor disturbances present. The color profile suggests a relatively evolved stellar population, with a bias toward redder wavelengths, although blue light is apparent.
