The galaxy presents as a spiral with a moderately inclined disk. A central bulge is visible, appearing yellow-white in color, suggesting an older stellar population. The disk exhibits a bluer hue, indicative of ongoing star formation within its spiral arms. Evidence of prominent spiral arm structure is noted, with a relatively tightly wound morphology. A weak bar may be present, bisecting the central bulge region. The overall structure appears relatively undisturbed with no signs of major mergers or tidal disruptions, although minor disturbances cannot be ruled out.
