The galaxy presents as a lenticular or possibly an elliptical type, with a notable absence of defined spiral arms. Its overall shape is elongated, appearing cigar-shaped, with a smooth, diffuse light distribution. The central bulge region exhibits a reddish hue, suggestive of an older stellar population, indicative of reduced star formation activity. The outer regions display a bluer color, implying the presence of younger stars. The light is concentrated towards the center and gradually fades into the background sky. There may be evidence of a minor disturbance, although the galaxy appears largely undisturbed, with no obvious signs of a recent major merger event.
