The galaxy presents as a slightly elongated, lenticular or early-type spiral galaxy with a smooth, centrally concentrated bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. Faint, diffuse blue light extends from the bulge, potentially suggesting the presence of some younger stars and ongoing, albeit modest, star formation within a nascent disk component. 

The overall shape appears somewhat irregular, with hints of subtle disturbances in the outer regions. These irregularities may be indicative of past minor merger events or gravitational interactions. No distinct spiral arm structure is immediately apparent. Based on its redshift, this galaxy is a relatively distant object, and its absolute magnitude suggests a galaxy of intermediate luminosity.
