The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with a high degree of central concentration. The overall shape is somewhat elongated, deviating from a perfectly circular form. There is no obvious disk component or spiral arm structure. The galaxy appears to be relatively isolated with only minor signs of tidal disturbance or interaction with other galaxies. The color indices suggest the presence of an older stellar population within the galaxy, though it is not entirely quiescent with evidence of recent or ongoing star formation. Given the redshift, the galaxy is at a considerable distance, therefore subtle features are difficult to resolve.
