The galaxy presents an elongated morphology, suggestive of a disk-like structure viewed at an oblique angle. A central bulge is visible, exhibiting a yellowish hue, possibly indicating an older stellar population dominating the core. The disk component shows some evidence of spiral arm structure, though it appears somewhat disrupted or flocculent. The color gradient across the disk indicates the presence of a relatively low level of recent star formation, with bluer regions sparsely distributed. A faint tidal tail or bridge appears to extend from one end of the galaxy, hinting at a past or ongoing gravitational interaction with another galaxy. The overall appearance indicates a massive galaxy with a moderate rate of star formation, potentially experiencing a minor interaction.
