The galaxy presents a notably elongated, cigar-shaped morphology. Its color is a gradient, appearing more yellowish-orange towards the central region and transitioning to a faint bluish hue at the outer edges. The smooth and diffuse light distribution suggests a relatively evolved stellar population, particularly in the galaxy's core. There are no clearly defined spiral arms or prominent dust lanes visible. The overall structure suggests a limited amount of ongoing star formation. There is no clear evidence of any major merger activity or tidal disturbances.
