The galaxy presents as a disk-shaped structure, exhibiting a relatively smooth morphology. A subtle central bulge is visible, with a diffuse glow emanating outwards. The disk displays a mottled texture, potentially indicative of spiral arm fragments or irregular dust lane distribution. The light is bluer in the outer disk, suggesting ongoing star formation, while the central bulge appears more yellow or red-shifted. The overall structure appears undisturbed, with no obvious signs of major tidal interactions or ongoing mergers, although a slight irregularity in the disk could indicate a minor interaction.
