The galaxy presents as an elongated, cigar-shaped structure. The central region displays a concentrated, bright yellowish-orange hue, suggesting an older stellar population and potentially higher dust content. Fainter bluish tinges appear toward the outer edges of the galaxy. This may indicate regions of ongoing star formation or a younger stellar population. The galaxy exhibits a relatively smooth texture overall, with no obvious spiral arm structures. A slight distortion or asymmetry is present along its major axis, which might suggest a minor gravitational interaction or disturbance. It is observed to be a larger galaxy, which likely resides at an intermediate distance based on its red shift.
