The galaxy exhibits a prominent disk structure, clearly viewed face-on. Spiral arms are distinctly visible, tracing a pattern from the central bulge outwards. The winding of these arms appears to be of medium tightness, with primarily two clearly defined arms dominating the structure. A moderate bulge is present in the center, exhibiting a yellowish hue suggestive of an older stellar population. The disk shows a bluer tint indicative of ongoing star formation, particularly within the spiral arms. There is a hint of a bar-like structure crossing the central region. No significant signs of major mergers or tidal disturbances are immediately apparent, though minor asymmetries may be present. Overall, the galaxy presents as a well-formed spiral galaxy with active star formation regions and a defined central bulge.
