The galaxy presents as a smooth, elongated structure, approximately 4.4 kpc in radius. Its morphology is largely featureless, appearing elliptical in shape with a high degree of symmetry. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer edges. There are no visually apparent spiral arms or prominent dust lanes. The color of the galaxy appears to be on the bluer side which may indicate ongoing star formation activity. There are no signs of a major merger, though a slight asymmetry might suggest a minor interaction or disturbance in its past or present.
