The galaxy presents a lenticular or possibly early-type spiral morphology. Its overall shape is a flattened ellipse, exhibiting a moderate degree of oblateness. The central bulge region appears smooth and moderately bright, with a color gradient suggesting an older stellar population. 

A faint disk is visible, extending outwards from the bulge. It appears relatively smooth with no prominent spiral arm structure, giving rise to a lenticular classification, but could also be tightly wound spiral arms which are not easily discernible in the image. The lack of distinct HII regions or dust lanes suggests a low rate of current star formation within the disk, although the blueish colouration of the disk, may suggest the presence of younger stars.

There is no visible evidence of ongoing major mergers or tidal interactions. The galaxy appears relatively undisturbed and isolated. Its photometric redshift indicates that it lies at a considerable distance. Based on the observed colors, luminosity, and morphology, it is likely a moderately massive galaxy with a relatively low specific star formation rate.
