The galaxy appears to be a relatively luminous spiral galaxy, exhibiting a moderate redshift. The central bulge is prominent and displays a yellowish-orange hue, suggestive of an older stellar population. The disk is somewhat elongated, possibly indicating an elliptical shape, but lacks well-defined spiral arms. The disk component presents a bluer color than the bulge, indicating the presence of younger, hotter stars, and thus ongoing star formation. Overall, the galaxy seems to be in a relatively quiescent state with potentially weak signs of interaction, it presents a smooth appearance with only slight irregularities in its morphology. The galaxy may be experiencing a minor disturbance or past merger event, as suggested by a slightly asymmetrical shape.
