The galaxy presents as a moderately bright, elongated system. Its overall shape is notably cigar-shaped, with a high degree of asymmetry, possibly indicating past or ongoing interactions. The galaxy exhibits a smooth, relatively featureless central bulge that appears nearly spherical, with a color gradient from a yellow-orange center to a bluer hue in the outer regions. This suggests an aging stellar population concentrated within the core. The disk component appears diffuse and displays very few distinct spiral arm structures. The blue color in the outer regions of the disk suggests the presence of some on-going star formation. There is no evidence of strong tidal features, such as prominent tails or bridges, to suggest a recent major merger event. Any disturbances observed appear subtle, more consistent with minor interactions or internal processes affecting the galaxy's morphology.
