The galaxy appears to be a relatively small, distant system with a moderate redshift. Morphologically, it is classified as a smooth galaxy with an elongated, cigar-shaped profile. The central region exhibits a high degree of spheroidal symmetry, with a gradual decrease in luminosity towards the outer edges. There is a subtle color gradient observed, transitioning from a bluer hue in the central region to redder tones in the outer portions of the galaxy, which could suggest differences in stellar populations and age. There is a subtle disturbance in the morphology, though it does not appear to be undergoing a major merging event. The overall structure suggests an elliptical morphology rather than a spiral. There is an even light distribution throughout the galaxy which lacks prominent features such as spiral arms or dust lanes.
