The galaxy presents as a somewhat smooth, elongated object with a concentrated central bulge. It exhibits a yellowish-orange hue throughout its structure, which could indicate an older stellar population. There is minimal evidence of distinct spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of ongoing major merger activity, although minor disturbances in the outer regions cannot be ruled out based on this image alone. The galaxy's morphology suggests a possible transition between a spiral and an elliptical type. The light is more intense from the middle, gently dispersed outwards to a halo that is less intensive.