The galaxy presents a disk-like morphology with a relatively bright, concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Faint, tightly wound spiral arms extend outwards from the bulge region. The spiral structure appears somewhat flocculent and less defined, and the overall color of the disk is more blueish, potentially indicating ongoing star formation. There is no strong evidence of a central bar structure. The galaxy is tilted with respect to our line of sight, presenting an elongated profile. No significant merging or tidal features are readily apparent, though the galaxy shows some minor distortions.
