The galaxy presents as a moderately luminous, distant object with an estimated redshift suggesting substantial cosmological distance. Morphologically, it appears to be a relatively smooth system, exhibiting characteristics consistent with an elliptical galaxy or a lenticular galaxy seen at low resolution. There is a slight elongation present, suggesting it is not perfectly spherical.

The galaxy appears to have a dominant central bulge, with a smooth transition in brightness outward from the core. There is little evidence of significant disk structure or spiral arms, indicating a lack of active star formation on a large scale. The color indices suggest a population of older stars. Given the smoothness and lack of significant tidal features, it is likely that the galaxy has either already completed any major mergers or is in a quiescent state following such events. Faint irregularities in the light distribution cannot be ruled out, however, the low resolution makes any accurate description difficult.
