The galaxy presents as a relatively smooth, disk-shaped structure. It exhibits a noticeable flattening, appearing elongated with an axial ratio of approximately 0.63. The primary color is a warm yellow-orange, concentrated towards the galaxy's center, suggesting an older stellar population dominates the core. Fainter blue-ish hues are present in the outer regions of the disk, possibly indicative of ongoing star formation or a younger stellar population in the spiral arms. There is no definitive evidence of a distinct spiral arm structure. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions.