This galaxy presents as an elongated structure, likely a disk-like system viewed at an oblique angle. The central region exhibits a concentrated, brighter core suggestive of either a significant bulge component or an active galactic nucleus, though without spectral data, this is speculative.

The color gradient transitions from a yellowish-white core to more reddish hues towards the outer edges. This reddening could indicate older stellar populations in the outer disk or the presence of dust obscuration. There appears to be limited evidence of distinct spiral arm structures within the visible portion of the galaxy. The overall smoothness of the light distribution suggests the galaxy is a relatively evolved system, possibly an early-type spiral or lenticular galaxy.

There may be evidence of a minor interaction or recent merger event, possibly with a smaller object nearby, based on asymmetries within the light distribution. The galaxy is relatively compact based on its angular size and the distance implied by its redshift.
