The object appears to be a galaxy at an intermediate redshift. It presents a generally smooth morphology with a high degree of central concentration, with little in the way of resolved substructure. Its shape is roughly round, exhibiting minimal elongation or distortion. There is no evidence of any ongoing major or minor mergers, or significant tidal disturbances. The galaxy's color profile suggests an older stellar population, with redder colors dominating the integrated light. This suggests that the galaxy may be dominated by older, lower-mass stars, and potentially has a relatively low current star formation rate.
