The galaxy presents a generally smooth morphology, with a notable absence of distinct spiral arms or prominent star-forming regions. The light distribution suggests an elliptical or lenticular type. The shape is elongated, appearing cigar-shaped, rather than perfectly spherical. The central region exhibits a concentration of light that fades gradually outward. No signs of ongoing major merging events are apparent. The galaxy displays a redder hue overall. There may be minor signs of disturbance.
